id string | question string | answer string | documents list |
|---|---|---|---|
10245_Inselsberg_31744821 | What does the article about '10245 Inselsberg' say regarding 'Naming'? | This minor planet was named after Großer Inselsberg, a mountain with an altitude of 916.5 m located in the Thuringian Forest in Thuringia, Germany. The official naming citation was published by the Minor Planet Center on 1 May 2003 (M.P.C. 48390). | [
"10245 Inselsberg — Naming\n\nThis minor planet was named after Großer Inselsberg, a mountain with an altitude of 916.5 m located in the Thuringian Forest in Thuringia, Germany. The official naming citation was published by the Minor Planet Center on 1 May 2003 (M.P.C. 48390).",
"10245 Inselsberg — Physical chara... |
10245_Inselsberg_31744819 | Explain what '10245 Inselsberg' covers in the 'Physical characteristics' section. | As a member of the Gefion family, Inselsberg is likely a stony S-type asteroid. It has an absolute magnitude of 13.2. As of 2018, no rotational lightcurve of Inselsberg has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown. | [
"10245 Inselsberg — Naming\n\nThis minor planet was named after Großer Inselsberg, a mountain with an altitude of 916.5 m located in the Thuringian Forest in Thuringia, Germany. The official naming citation was published by the Minor Planet Center on 1 May 2003 (M.P.C. 48390).",
"10245 Inselsberg — Physical chara... |
10245_Inselsberg_31744817 | Summarize the 'Orbit and classification' part of '10245 Inselsberg'. | Inselsberg is a member of the Gefion family (516), a large intermediate belt family, named after 1272 Gefion It orbits the Sun in the central asteroid belt at a distance of 2.5–3.0 AU once every 4 years and 8 months (1,695 days; semi-major axis of 2.78 AU). Its orbit has an eccentricity of 0.09 and an inclination of 9°... | [
"10245 Inselsberg — Naming\n\nThis minor planet was named after Großer Inselsberg, a mountain with an altitude of 916.5 m located in the Thuringian Forest in Thuringia, Germany. The official naming citation was published by the Minor Planet Center on 1 May 2003 (M.P.C. 48390).",
"10245 Inselsberg — Physical chara... |
10245_Inselsberg_31744818 | Based on the article about '10245 Inselsberg', describe the 'Palomar–Leiden survey' section. | The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingr... | [
"10245 Inselsberg — Naming\n\nThis minor planet was named after Großer Inselsberg, a mountain with an altitude of 916.5 m located in the Thuringian Forest in Thuringia, Germany. The official naming citation was published by the Minor Planet Center on 1 May 2003 (M.P.C. 48390).",
"10245 Inselsberg — Physical chara... |
10245_Inselsberg_31744820 | Based on the article about '10245 Inselsberg', describe the 'Diameter and albedo' section. | Based on a generic magnitude-to-diameter conversion, Inselsberg measures 6.9 kilometers in diameter for an assumed stony albedo of 0.20, derived from the Gefion family's standard albedo, and a measured absolute magnitude of 13.2. According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared S... | [
"10245 Inselsberg — Naming\n\nThis minor planet was named after Großer Inselsberg, a mountain with an altitude of 916.5 m located in the Thuringian Forest in Thuringia, Germany. The official naming citation was published by the Minor Planet Center on 1 May 2003 (M.P.C. 48390).",
"10245 Inselsberg — Physical chara... |
10247_Amphiaraos_31368312 | Explain what '10247 Amphiaraos' covers in the 'Naming' section. | This minor planet was named after the Greek seer Amphiaraus (Amphiaraos), who was the king of Argos. He was one of the Seven against Thebes. The official was published by the Minor Planet Center on 24 January 2000 (M.P.C. 38199). | [
"10247 Amphiaraos — Naming\n\nThis minor planet was named after the Greek seer Amphiaraus (Amphiaraos), who was the king of Argos. He was one of the Seven against Thebes. The official was published by the Minor Planet Center on 24 January 2000 (M.P.C. 38199).",
"10247 Amphiaraos — Physical characteristics\n\nAmph... |
10247_Amphiaraos_31368309 | What does the article about '10247 Amphiaraos' say regarding 'Physical characteristics'? | Amphiaraos has been characterized as an X and D-type asteroid in the SDSS-based taxonomy, and by Pan-STARRS' survey. It is also an assumed C-type. | [
"10247 Amphiaraos — Naming\n\nThis minor planet was named after the Greek seer Amphiaraus (Amphiaraos), who was the king of Argos. He was one of the Seven against Thebes. The official was published by the Minor Planet Center on 24 January 2000 (M.P.C. 38199).",
"10247 Amphiaraos — Physical characteristics\n\nAmph... |
10247_Amphiaraos_31368306 | Summarize the following section from the article on '10247 Amphiaraos'. | 10247 Amphiaraos is Jupiter trojan from the Greek camp, approximately 27 km in diameter. It was discovered on 24 September 1960, by Dutch astronomers Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at the Palomar Observatory in California. The X/D-type asteroid has a long rotation period of 34.26 hours and po... | [
"10247 Amphiaraos — Naming\n\nThis minor planet was named after the Greek seer Amphiaraus (Amphiaraos), who was the king of Argos. He was one of the Seven against Thebes. The official was published by the Minor Planet Center on 24 January 2000 (M.P.C. 38199).",
"10247 Amphiaraos — Physical characteristics\n\nAmph... |
10247_Amphiaraos_31368308 | From the article on '10247 Amphiaraos', restate the 'Palomar–Leiden survey' content. | The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingr... | [
"10247 Amphiaraos — Naming\n\nThis minor planet was named after the Greek seer Amphiaraus (Amphiaraos), who was the king of Argos. He was one of the Seven against Thebes. The official was published by the Minor Planet Center on 24 January 2000 (M.P.C. 38199).",
"10247 Amphiaraos — Physical characteristics\n\nAmph... |
10247_Amphiaraos_31368310 | Based on the article about '10247 Amphiaraos', describe the 'Rotation period' section. | In March 2012, a rotational lightcurve of Amphiaraos was obtained from photometric observations by Robert Stephens, Daniel Coley and Ralph Megna at the Goat Mountain Astronomical Research Station in California. Lightcurve analysis gave a longer-than average rotation period of 34.26 hours with a brightness amplitude of ... | [
"10247 Amphiaraos — Naming\n\nThis minor planet was named after the Greek seer Amphiaraus (Amphiaraos), who was the king of Argos. He was one of the Seven against Thebes. The official was published by the Minor Planet Center on 24 January 2000 (M.P.C. 38199).",
"10247 Amphiaraos — Physical characteristics\n\nAmph... |
10247_Amphiaraos_31368307 | Summarize the 'Orbit and classification' part of '10247 Amphiaraos'. | Amphiaraos is a Jovian asteroid orbiting in the leading Greek camp at Jupiter's Lagrangian point, 60° ahead of the Gas Giant's orbit in a 1:1 resonance (see Trojans in astronomy). It is a non-family asteroid in the Jovian background population. It orbits the Sun at a distance of 5.2–5.3 AU once every 12 years and 1 mon... | [
"10247 Amphiaraos — Naming\n\nThis minor planet was named after the Greek seer Amphiaraus (Amphiaraos), who was the king of Argos. He was one of the Seven against Thebes. The official was published by the Minor Planet Center on 24 January 2000 (M.P.C. 38199).",
"10247 Amphiaraos — Physical characteristics\n\nAmph... |
10249_Harz_31744199 | What information does the article about '10249 Harz' provide on 'Palomar–Leiden survey'? | The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingr... | [
"10249 Harz — Palomar–Leiden survey\n\nThe survey designation \"P-L\" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope)... |
10249_Harz_31744200 | Describe the 'Physical characteristics' section of the article about '10249 Harz'. | Harz is an assumed S-type asteroid, which agrees with the measured albedo (see below) by the Wide-field Infrared Survey Explorer (WISE). | [
"10249 Harz — Palomar–Leiden survey\n\nThe survey designation \"P-L\" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope)... |
10249_Harz_31744202 | Based on the article about '10249 Harz', describe the 'Diameter and albedo' section. | According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Harz measures between 3.59 kilometers in diameter and its surface has an albedo of 0.26, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.15 kilometer... | [
"10249 Harz — Palomar–Leiden survey\n\nThe survey designation \"P-L\" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope)... |
10249_Harz_31744198 | Based on the article about '10249 Harz', describe the 'Orbit and classification' section. | Harz is a non-family asteroid from the main belt's background population. It orbits the Sun in the central main-belt at a distance of 2.3–2.8 AU once every 4 years and 2 months (1,510 days; semi-major axis of 2.58 AU). Its orbit has an eccentricity of 0.09 and an inclination of 4° with respect to the ecliptic. The body... | [
"10249 Harz — Palomar–Leiden survey\n\nThe survey designation \"P-L\" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope)... |
10249_Harz_31744197 | Summarize the following section from the article on '10249 Harz'. | 10249 Harz, provisional designation, is a background asteroid from the central regions of the asteroid belt, approximately 3.5 km in diameter. It was discovered on 17 October 1960, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observatory in California, United States. The assumed S-type astero... | [
"10249 Harz — Palomar–Leiden survey\n\nThe survey designation \"P-L\" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope)... |
10249_Harz_31744203 | What does the article about '10249 Harz' say regarding 'Naming'? | This minor planet was named after the Harz mountains, an old German mountain range where silver was mined until the last century. Legend has it that the witches gathered on their broomsticks on a plateau in the Harz mountains on the first day of May. The legendary place where the witches danced is known as Hexentanzpla... | [
"10249 Harz — Palomar–Leiden survey\n\nThe survey designation \"P-L\" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope)... |
10249_Harz_31744201 | Reconstruct the content about 'Rotation period' from the article on '10249 Harz'. | In October 2010, and December 2014, two rotational lightcurves of Harz were obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 3.631 and 3.64 hours with a brightness amplitude of 0.47 and 0.52 magnitude, respe... | [
"10249 Harz — Palomar–Leiden survey\n\nThe survey designation \"P-L\" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope)... |
1025_25493360 | Explain what '1025' covers in the 'Deaths' section. | June 17 – Bolesław I the Brave, king of Poland (b. 967) ; September 17 – Hugh Magnus, king of France (b. 1007) ; September 29 – Louis I, count of Chiny and Verdun ; December 15 – Basil II, Byzantine emperor (b. 958) ; December 22 – Wang Qinruo, Chinese chancellor ; Abd al-Jabbar ibn Ahmad,... | [
"1025 — Deaths\n\nJune 17 – Bolesław I the Brave, king of Poland (b. 967) ; September 17 – Hugh Magnus, king of France (b. 1007) ; September 29 – Louis I, count of Chiny and Verdun ; December 15 – Basil II, Byzantine emperor (b. 958) ; December 22 – Wang Qinruo, Chinese chancellor ; Ab... |
1025_25493353 | What information does the article about '1025' provide? | Year 1025 (MXXV) was a common year starting on Friday (link will display the full calendar) of the Julian calendar. | [
"1025 — Deaths\n\nJune 17 – Bolesław I the Brave, king of Poland (b. 967) ; September 17 – Hugh Magnus, king of France (b. 1007) ; September 29 – Louis I, count of Chiny and Verdun ; December 15 – Basil II, Byzantine emperor (b. 958) ; December 22 – Wang Qinruo, Chinese chancellor ; Ab... |
1025_25493358 | What information does the article about '1025' provide on 'Asia'? | Srivijaya, a Buddhist kingdom based in Sumatra, is attacked by Emperor Rajendra I of the Chola dynasty of southern India in a dispute over trading rights in Southeast Asia. It survives, but declines in importance. ; Completion and publishing of Avicenna's Canon of Medicine | [
"1025 — Deaths\n\nJune 17 – Bolesław I the Brave, king of Poland (b. 967) ; September 17 – Hugh Magnus, king of France (b. 1007) ; September 29 – Louis I, count of Chiny and Verdun ; December 15 – Basil II, Byzantine emperor (b. 958) ; December 22 – Wang Qinruo, Chinese chancellor ; Ab... |
1025_25493354 | Based on the article about '1025', describe the 'Japan' section. | - Regent Yorimichi holds horse racing in his mansion (the emperor attends, too) 21 January: Daughter of Fujiwara no Sanesuke (rival of Michinaga), Chifuru has her Mogi Ceremony - Sanesuke want to make his daughter to imperial consort which cause the dislike of Empress Ishi (daughter of Michinaga) - eventually Regent Yo... | [
"1025 — Deaths\n\nJune 17 – Bolesław I the Brave, king of Poland (b. 967) ; September 17 – Hugh Magnus, king of France (b. 1007) ; September 29 – Louis I, count of Chiny and Verdun ; December 15 – Basil II, Byzantine emperor (b. 958) ; December 22 – Wang Qinruo, Chinese chancellor ; Ab... |
1025_25493356 | Explain what '1025' covers in the 'Europe' section. | April 18 – Bolesław I the Brave is crowned in Gniezno as the first king of Poland. He takes advantage of the interregnum in Germany (see 1024), and receives permission for his coronation from Pope John XIX; however, he dies on June 17. ; September – At the urging of Queen Constance of Arles, the three sons ... | [
"1025 — Deaths\n\nJune 17 – Bolesław I the Brave, king of Poland (b. 967) ; September 17 – Hugh Magnus, king of France (b. 1007) ; September 29 – Louis I, count of Chiny and Verdun ; December 15 – Basil II, Byzantine emperor (b. 958) ; December 22 – Wang Qinruo, Chinese chancellor ; Ab... |
1025_25493355 | Summarize the 'Byzantine Empire' part of '1025'. | December 15 – Byzantine Emperor Basil II ("Bulgar Slayer") dies in Constantinople after a 50-year reign. Never married, he is succeeded by his brother and co-emperor Constantine VIII who becomes sole ruler of the Byzantine Empire. Constantine calls the Sicilian invasion off. Catapan Basil Boioannes diverts the By... | [
"1025 — Deaths\n\nJune 17 – Bolesław I the Brave, king of Poland (b. 967) ; September 17 – Hugh Magnus, king of France (b. 1007) ; September 29 – Louis I, count of Chiny and Verdun ; December 15 – Basil II, Byzantine emperor (b. 958) ; December 22 – Wang Qinruo, Chinese chancellor ; Ab... |
1025_Riema_20699668 | From the article on '1025 Riema', restate the 'Lightcurves' content. | In August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2). The Ukrainian team also determined the body's poles... | [
"1025 Riema — Lightcurves\n\nIn August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2). The Ukrainian team... |
1025_Riema_20699669 | Reconstruct the content about 'Diameter and albedo' from the article on '1025 Riema'. | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Riema measures 4.605 kilometers in diameter and its surface has an outstandingly high albedo of 1.000. The Collaborative Asteroid Lightcurve Link assumes an albedo for E-type Hungaria asteroids of 0.40 – taken from... | [
"1025 Riema — Lightcurves\n\nIn August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2). The Ukrainian team... |
1025_Riema_20699667 | Based on the article about '1025 Riema', describe the 'Physical characteristics' section. | In the Tholen classification, Riema is a bright E-type asteroid. In the SMASS taxonomy, it has been classified as a Xe-type, which transitions from the E to the X-types. In addition, the asteroid has also been polarimetrically characterized as a metallic M-type asteroid. | [
"1025 Riema — Lightcurves\n\nIn August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2). The Ukrainian team... |
1025_Riema_20699665 | Reconstruct the content from the article about '1025 Riema'. | 1025 Riema, provisional designation, is a bright Hungaria asteroid from the innermost regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 12 August 1923, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The asteroid was named after ARI astrono... | [
"1025 Riema — Lightcurves\n\nIn August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2). The Ukrainian team... |
1025_Riema_20699670 | Explain what '1025 Riema' covers in the 'Naming' section. | This minor planet was named after Johannes Karl Richard Riem (1868–1945), a German astronomer at the Astronomisches Rechen-Institut (ARI) in Berlin. The name was suggested by ARI. The official naming citation was published by Paul Herget in The Names of the Minor Planets in 1955 (H 98). | [
"1025 Riema — Lightcurves\n\nIn August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2). The Ukrainian team... |
1025_Riema_20699666 | What information does the article about '1025 Riema' provide on 'Orbit and classification'? | Riema is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun at a distance of 1.9–2.1 AU once every 2 years and 9 months (1,017 days). Its orbit has an eccentricity of 0.04 and an inclination of 27° with respect to the ecliptic. The asteroid'... | [
"1025 Riema — Lightcurves\n\nIn August 2001, a first rotational lightcurve of Riema was obtained from photometric observations by Ukrainian astronomers at Kharkiv (101) and Simeiz (094). Lightcurve analysis gave a rotation period of 6.557 hours with a brightness variation of 0.25 magnitude (U=2). The Ukrainian team... |
1025_rally_to_safeguard_Taiwan_5513225 | Based on the article about '1025 rally to safeguard Taiwan', describe the 'Demonstration' section. | Because the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies, former President Chen Shui-bian also marched and took... | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
1025_rally_to_safeguard_Taiwan_5513226 | Summarize the 'Controversial officer' part of '1025 rally to safeguard Taiwan'. | When protesters asked a police officer whether her boss is President Ma or not, the officer, surnamed Chou, responded that she worked for the People's Republic of China (PRC). The response irritated pan-green supporters, and an apology was immediately demanded. Chou apologized and left the scene. The director of the Na... | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
1025_rally_to_safeguard_Taiwan_5513223 | Explain what '1025 rally to safeguard Taiwan' covers in the 'Parade routes' section. | "Oppose Toxic Goods" (approx. 3.9 km) ; "Oppose One China Education" (approx. 3.4 km) ; "Oppose the Hollowing Out of Sovereignty" (approx. 3.8 km) ; "Oppose a One China Market" (approx. 4.2 km) ; "Oppose the Incompetent Government" (approx. 4.8 km) The planned starting point of the first route "Oppose Toxic Goods" was... | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
1025_rally_to_safeguard_Taiwan_5513227 | What information does the article about '1025 rally to safeguard Taiwan' provide on 'Responses'? | President Ma Ying-jeou said he would listen to the voice of the people and respond to their criticism, but maintained that the main direction of his government policies remained the correct one. | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
1025_rally_to_safeguard_Taiwan_5513221 | Summarize the 'Cross-strait relations' part of '1025 rally to safeguard Taiwan'. | car that Zhang was in was attacked and damaged when a protester jumped on the top of the car. Later, Zhang remarked, "Those who commit violence do not get what they want, but instead drop a rock on their own feet." as well as "A handful of compatriots in Tainan were involved in the violence (against me). They do not re... | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
1025_rally_to_safeguard_Taiwan_5513224 | Reconstruct the content about 'Parade routes' from the article on '1025 rally to safeguard Taiwan'. | DPP chairwoman Tsai Ing-wen, former Kaohsiung mayor Yeh Chu-lan, current mayor Chen Chu, and Kaohsiung County magistrate Yang Chiu-hsing. The third route was organized by the TSU. Protesters marched from the Lungshan Temple. The TSU convened about 20,000 people including members of Victims of Investment in China Associ... | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
1025_rally_to_safeguard_Taiwan_5513220 | What information does the article about '1025 rally to safeguard Taiwan' provide on 'Cross-strait relations'? | The People's Republic of China claims that self-ruled Taiwan is its 23rd province. The PRC has threatened the use of force if Taiwan declares de jure independence from China. Zhang Mingqing, the deputy chairman of the Association for Relations Across the Taiwan Strait, arrived in Taiwan about a week before the protest.... | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
1025_rally_to_safeguard_Taiwan_5513219 | Reconstruct the content from the article about '1025 rally to safeguard Taiwan'. | The 1025 demonstration was a demonstration on 25 October 2008 sponsored by the Democratic Progressive Party (DPP) and Taiwan Solidarity Union in Taipei, Taiwan. This protest march was launched five months after the inauguration of President Ma Ying-jeou and was preceded by an earlier 30 August 2008 protest in August w... | [
"1025 rally to safeguard Taiwan — Demonstration\n\nBecause the protest march was launched primarily by the Democratic Progressive Party, participants were predominantly pan-green. Former DPP chairmen Yao Chia-wen, Su Tseng-chang, and Yu Shyi-kun all participated in the march. Despite recent corruption controversies... |
10251_Mulisch_27460642 | Summarize the 'Diameter and albedo' part of '10251 Mulisch'. | According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Mulisch measures 2.398 kilometers in diameter and its surface has an albedo of 0.337. | [
"10251 Mulisch — Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Mulisch measures 2.398 kilometers in diameter and its surface has an albedo of 0.337.",
"10251 Mulisch — Physical characteristics\n\nThe asteroid has an absolute magnitude 15.2. Based on it... |
10251_Mulisch_27460641 | Reconstruct the content about 'Physical characteristics' from the article on '10251 Mulisch'. | The asteroid has an absolute magnitude 15.2. Based on its high albedo measured by the Wide-field Infrared Survey Explorer, Mulisch likely belongs to the stony S-complex. As of 2018, no rotational lightcurve of this asteroid has been obtained from photometric observations. Its rotation period, pole and shape remain unkn... | [
"10251 Mulisch — Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Mulisch measures 2.398 kilometers in diameter and its surface has an albedo of 0.337.",
"10251 Mulisch — Physical characteristics\n\nThe asteroid has an absolute magnitude 15.2. Based on it... |
10251_Mulisch_27460640 | What does the article about '10251 Mulisch' say regarding 'Palomar–Leiden Trojan survey'? | The survey designation "T-1" stands for the first Palomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar and Leiden Observatory in the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid... | [
"10251 Mulisch — Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Mulisch measures 2.398 kilometers in diameter and its surface has an albedo of 0.337.",
"10251 Mulisch — Physical characteristics\n\nThe asteroid has an absolute magnitude 15.2. Based on it... |
10251_Mulisch_27460639 | Explain what '10251 Mulisch' covers in the 'Orbit and classification' section. | Mulisch is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner main-belt at a distance of 2.1–2.5 AU once every 3 years and 7 months (1,302 days; semi-major axis of 2.33 AU). Its orbit has an eccentricity of 0.09 and an inclination of 2° with respect to the ecliptic. The bod... | [
"10251 Mulisch — Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Mulisch measures 2.398 kilometers in diameter and its surface has an albedo of 0.337.",
"10251 Mulisch — Physical characteristics\n\nThe asteroid has an absolute magnitude 15.2. Based on it... |
10251_Mulisch_27460643 | From the article on '10251 Mulisch', restate the 'Naming' content. | This minor planet was named after Dutch writer Harry Mulisch (1927–2010), known for his novels, plays, essays, poems and philosophical reflections such as The Discovery of Heaven. The official naming citation was published by the Minor Planet Center on 13 June 2006 (M.P.C. 56959). | [
"10251 Mulisch — Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Mulisch measures 2.398 kilometers in diameter and its surface has an albedo of 0.337.",
"10251 Mulisch — Physical characteristics\n\nThe asteroid has an absolute magnitude 15.2. Based on it... |
10251_Mulisch_27460638 | Describe the content of the article about '10251 Mulisch'. | 10251 Mulisch, provisional designation, is a bright background asteroid from the inner regions of the asteroid belt, approximately 2.4 km in diameter. It was discovered during the Palomar–Leiden Trojan survey on 26 March 1971, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observatory in Califo... | [
"10251 Mulisch — Diameter and albedo\n\nAccording to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Mulisch measures 2.398 kilometers in diameter and its surface has an albedo of 0.337.",
"10251 Mulisch — Physical characteristics\n\nThe asteroid has an absolute magnitude 15.2. Based on it... |
10252_Heidigraf_23538450 | Reconstruct the content from the article about '10252 Heidigraf'. | 10252 Heidigraf, provisional designation, is a Koronian asteroid from the outer regions of the asteroid belt, approximately 6 km in diameter. It was discovered during the Palomar–Leiden Trojan survey on 26 March 1971, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observatory in California, Uni... | [
"10252 Heidigraf\n\n10252 Heidigraf, provisional designation, is a Koronian asteroid from the outer regions of the asteroid belt, approximately 6 km in diameter. It was discovered during the Palomar–Leiden Trojan survey on 26 March 1971, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observ... |
10252_Heidigraf_23538456 | Based on the article about '10252 Heidigraf', describe the 'Naming' section. | This minor planet was named after Heidi Graf (born 1941), former Head of the European Space Research and Technology Centre (ESTEC) Communications Office from 1977 to 2006 at the European Space Agency, ESA. The official naming citation was published by the Minor Planet Center on 9 November 2006 (M.P.C. 57950). | [
"10252 Heidigraf\n\n10252 Heidigraf, provisional designation, is a Koronian asteroid from the outer regions of the asteroid belt, approximately 6 km in diameter. It was discovered during the Palomar–Leiden Trojan survey on 26 March 1971, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observ... |
10252_Heidigraf_23538455 | What information does the article about '10252 Heidigraf' provide on 'Diameter and albedo'? | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Heidigraf measures 5.782 kilometers in diameter and its surface has an albedo of 0.331 and 0.4007, respectively. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 and calculates a diameter of 5.1... | [
"10252 Heidigraf\n\n10252 Heidigraf, provisional designation, is a Koronian asteroid from the outer regions of the asteroid belt, approximately 6 km in diameter. It was discovered during the Palomar–Leiden Trojan survey on 26 March 1971, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observ... |
10252_Heidigraf_23538452 | What information does the article about '10252 Heidigraf' provide on 'Palomar–Leiden Trojan survey'? | The survey designation "T-1" stands for the first Palomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar and Leiden Observatory in the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid... | [
"10252 Heidigraf\n\n10252 Heidigraf, provisional designation, is a Koronian asteroid from the outer regions of the asteroid belt, approximately 6 km in diameter. It was discovered during the Palomar–Leiden Trojan survey on 26 March 1971, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observ... |
10258_Sárneczky_5673774 | What information does the article about '10258 Sárneczky' provide on 'Rotation period'? | As of 2017, no rotational lightcurve of Sárneczky has been obtained from photometric observations. The body's rotation period, shape and poles remain unknown. | [
"10258 Sárneczky — Rotation period\n\nAs of 2017, no rotational lightcurve of Sárneczky has been obtained from photometric observations. The body's rotation period, shape and poles remain unknown.",
"10258 Sárneczky — Naming\n\nThis minor planet was named after Krisztián Sárneczky (born 1974), a Hungarian amateur... |
10258_Sárneczky_5673775 | Reconstruct the content about 'Naming' from the article on '10258 Sárneczky'. | This minor planet was named after Krisztián Sárneczky (born 1974), a Hungarian amateur astronomer and discoverer of minor planets and supernovae. He is a board member of the Hungarian Astronomical Association (HAA). The official naming citation was published by the Minor Planet Center on 5 October 2017 (M.P.C. 106499). | [
"10258 Sárneczky — Rotation period\n\nAs of 2017, no rotational lightcurve of Sárneczky has been obtained from photometric observations. The body's rotation period, shape and poles remain unknown.",
"10258 Sárneczky — Naming\n\nThis minor planet was named after Krisztián Sárneczky (born 1974), a Hungarian amateur... |
10258_Sárneczky_5673772 | Based on the article about '10258 Sárneczky', describe the 'Orbit and classification' section. | Sárneczky is non-family asteroid from the main-belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.5 AU once every 5 years and 7 months (2,053 days). Its orbit has an eccentricity of 0.09 and an inclination of 14° with respect to the ecliptic. The body's observation arc beg... | [
"10258 Sárneczky — Rotation period\n\nAs of 2017, no rotational lightcurve of Sárneczky has been obtained from photometric observations. The body's rotation period, shape and poles remain unknown.",
"10258 Sárneczky — Naming\n\nThis minor planet was named after Krisztián Sárneczky (born 1974), a Hungarian amateur... |
10258_Sárneczky_5673771 | Summarize the following section from the article on '10258 Sárneczky'. | 10258 Sárneczky, provisional designation, is a background asteroid from the outer regions of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 6 January 1940, by Hungarian astronomer György Kulin at the Konkoly Observatory, near Budapest. The asteroid was named after Hungarian astronomer ... | [
"10258 Sárneczky — Rotation period\n\nAs of 2017, no rotational lightcurve of Sárneczky has been obtained from photometric observations. The body's rotation period, shape and poles remain unknown.",
"10258 Sárneczky — Naming\n\nThis minor planet was named after Krisztián Sárneczky (born 1974), a Hungarian amateur... |
1026_25112013 | Based on the article about '1026', describe the 'Deaths' section. | June 10 – Hugh II, French viscount and archbishop ; August 28 – Richard II, "the Good", duke of Normandy ; August 30 – Bononio, Lombard hermit and abbot ; September 21 – Otto-William, count of Burgundy ; November 27 – Adalbold II, bishop of Utrecht ; Adelaide-Blanche of Anjou, French queen... | [
"1026 — Deaths\n\nJune 10 – Hugh II, French viscount and archbishop ; August 28 – Richard II, \"the Good\", duke of Normandy ; August 30 – Bononio, Lombard hermit and abbot ; September 21 – Otto-William, count of Burgundy ; November 27 – Adalbold II, bishop of Utrecht ; Adelaide-Blanch... |
1026_25112008 | What information does the article about '1026' provide? | Year 1026 (MXXVI) was a common year starting on Saturday (link will display the full calendar) of the Julian calendar. | [
"1026 — Deaths\n\nJune 10 – Hugh II, French viscount and archbishop ; August 28 – Richard II, \"the Good\", duke of Normandy ; August 30 – Bononio, Lombard hermit and abbot ; September 21 – Otto-William, count of Burgundy ; November 27 – Adalbold II, bishop of Utrecht ; Adelaide-Blanch... |
1026_25112009 | Describe the 'Europe' section of the article about '1026'. | Spring – King Conrad II, "the Elder", assembles an army of thousands of armored knights for an expedition into Italy. He besieges Pavia and marches to Milan, where he is crowned with the Iron Crown by Archbishop Aribert as king of the Lombards. Duke William V ("the Great") of Aquitaine, who is already en route fo... | [
"1026 — Deaths\n\nJune 10 – Hugh II, French viscount and archbishop ; August 28 – Richard II, \"the Good\", duke of Normandy ; August 30 – Bononio, Lombard hermit and abbot ; September 21 – Otto-William, count of Burgundy ; November 27 – Adalbold II, bishop of Utrecht ; Adelaide-Blanch... |
1026_25112012 | Based on the article about '1026', describe the 'Births' section. | Lidanus, Lombard Benedictine abbot (d. 1118) ; Tostig Godwinson, earl of Northumbria (approximate date) ; Pope Victor III, born Dauferio, Lombard churchman (approximate date) ; William Firmatus, Norman hermit and pilgrim (d. 1103) | [
"1026 — Deaths\n\nJune 10 – Hugh II, French viscount and archbishop ; August 28 – Richard II, \"the Good\", duke of Normandy ; August 30 – Bononio, Lombard hermit and abbot ; September 21 – Otto-William, count of Burgundy ; November 27 – Adalbold II, bishop of Utrecht ; Adelaide-Blanch... |
1026_25112011 | What does the article about '1026' say regarding 'Asia'? | A Zubu revolt against the Liao dynasty is suppressed, with the Zubu forced to pay an annual tribute of horses, camels and furs. | [
"1026 — Deaths\n\nJune 10 – Hugh II, French viscount and archbishop ; August 28 – Richard II, \"the Good\", duke of Normandy ; August 30 – Bononio, Lombard hermit and abbot ; September 21 – Otto-William, count of Burgundy ; November 27 – Adalbold II, bishop of Utrecht ; Adelaide-Blanch... |
1026_25112010 | Based on the article about '1026', describe the 'Europe' section. | and takes Ravenna, taking bloody revenge. ; 1 June – The Basilica of Saint Maternus in Walcourt, present-day Belgium, is consecrated by Bishop Réginhard of Liège. ; Conrad II proceeds to Pesaro, but a malarian outbreak forces him to withdraw back up north to the Po Valley. He subdues the March of Turin, where Cou... | [
"1026 — Deaths\n\nJune 10 – Hugh II, French viscount and archbishop ; August 28 – Richard II, \"the Good\", duke of Normandy ; August 30 – Bononio, Lombard hermit and abbot ; September 21 – Otto-William, count of Burgundy ; November 27 – Adalbold II, bishop of Utrecht ; Adelaide-Blanch... |
1026_Ingrid_21323212 | Summarize the 'Naming' part of '1026 Ingrid'. | This minor planet was named after Ingrid, niece and godchild of Albrecht Kahrstedt (1897–1971), a German astronomer at ARI and director of the institute's Potsdam division, who requested the naming of this asteroid and 984 Gretia (mother of Ingrid) in a personal letter to the discoverer in February 1926. Kahrstedt hims... | [
"1026 Ingrid — Naming\n\nThis minor planet was named after Ingrid, niece and godchild of Albrecht Kahrstedt (1897–1971), a German astronomer at ARI and director of the institute's Potsdam division, who requested the naming of this asteroid and 984 Gretia (mother of Ingrid) in a personal letter to the discoverer in ... |
1026_Ingrid_21323208 | Reconstruct the content about 'Orbit and classification' from the article on '1026 Ingrid'. | Ingrid is a member of the Flora family (402), a giant asteroid family and the largest family of stony asteroids. It orbits the Sun in the inner main-belt at a distance of 1.8–2.7 AU once every 3 years and 5 months (1,237 days). Its orbit has an eccentricity of 0.18 and an inclination of 5° with respect to the ecliptic.... | [
"1026 Ingrid — Naming\n\nThis minor planet was named after Ingrid, niece and godchild of Albrecht Kahrstedt (1897–1971), a German astronomer at ARI and director of the institute's Potsdam division, who requested the naming of this asteroid and 984 Gretia (mother of Ingrid) in a personal letter to the discoverer in ... |
1026_Ingrid_21323210 | From the article on '1026 Ingrid', restate the 'Rotation period' content. | A rotational lightcurve of Ingrid was obtained from photometric observations by a group of Hungarian astronomers. The 2005-published lightcurve analysis gave a rotation period of 5 hours with a brightness variation of 0.5 magnitude (U=2). | [
"1026 Ingrid — Naming\n\nThis minor planet was named after Ingrid, niece and godchild of Albrecht Kahrstedt (1897–1971), a German astronomer at ARI and director of the institute's Potsdam division, who requested the naming of this asteroid and 984 Gretia (mother of Ingrid) in a personal letter to the discoverer in ... |
1026_Ingrid_21323206 | What information does the article about '1026 Ingrid' provide? | 1026 Ingrid, provisional designation, is a stony Florian asteroid and long-lost minor planet (1923–1986) from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by Karl Reinmuth at Heidelberg in 1923, and later named after Ingrid, niece and godchild of astronomer Albrecht ... | [
"1026 Ingrid — Naming\n\nThis minor planet was named after Ingrid, niece and godchild of Albrecht Kahrstedt (1897–1971), a German astronomer at ARI and director of the institute's Potsdam division, who requested the naming of this asteroid and 984 Gretia (mother of Ingrid) in a personal letter to the discoverer in ... |
1026_Ingrid_21323211 | What does the article about '1026 Ingrid' say regarding 'Diameter and albedo'? | According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Ingrid measures between 5.73 and 7.67 kilometers in diameter and its surface has an albedo between 0.1441 and 0.43. The Collaborative Asteroid Lightcurve Link assumes an albedo of ... | [
"1026 Ingrid — Naming\n\nThis minor planet was named after Ingrid, niece and godchild of Albrecht Kahrstedt (1897–1971), a German astronomer at ARI and director of the institute's Potsdam division, who requested the naming of this asteroid and 984 Gretia (mother of Ingrid) in a personal letter to the discoverer in ... |
1026_Ingrid_21323207 | Based on the article about '1026 Ingrid', describe the 'Discovery and recovery' section. | Ingrid was discovered on 13 August 1923, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was observed for only a few days during August 1923, before it became a lost minor planet for nearly 63 years until its recovery by Japanese astronomer Syuichi Na... | [
"1026 Ingrid — Naming\n\nThis minor planet was named after Ingrid, niece and godchild of Albrecht Kahrstedt (1897–1971), a German astronomer at ARI and director of the institute's Potsdam division, who requested the naming of this asteroid and 984 Gretia (mother of Ingrid) in a personal letter to the discoverer in ... |
1027_26474754 | What information does the article about '1027' provide? | Year 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar. | [
"1027\n\nYear 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar.",
"1027 — Births\n\nAlbert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. ... |
1027_26474759 | What does the article about '1027' say regarding 'Births'? | Albert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. 1075) ; Fayun Faxiu, Chinese Chan Buddhist monk (d. 1090) ; Matilda of Franconia, German princess (d. 1034) ; Shōshi, Japanese empress consort (d. 1105) ... | [
"1027\n\nYear 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar.",
"1027 — Births\n\nAlbert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. ... |
1027_26474760 | What does the article about '1027' say regarding 'Deaths'? | January 3 – Fujiwara no Yukinari, Japanese calligrapher (b. 972) ; August 6 – Richard III, duke of Normandy (House of Normandy) ; August 16 – George I, king of Georgia (House of Bagrationi) ; October 16 – Fujiwara no Kenshi, Japanese empress (b. 994) ; Abu'l-Qasim al-Husayn ibn Ali al-Maghribi, ... | [
"1027\n\nYear 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar.",
"1027 — Births\n\nAlbert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. ... |
1027_26474758 | Based on the article about '1027', describe the 'Science, technology and medicine' section. | The Book of Healing (Arabic: کتاب الشفاء Kitab Al-Shifaʾ, Latin: Sufficientia), a comprehensive scientific and philosophical encyclopedia written by the Persian polymath Avicenna (Abū ʿAlī ibn Sīnā), is published. ; Song dynasty Chinese engineer Yan Su reinvents the 3rd-century south-pointing chariot, a mechanical-driv... | [
"1027\n\nYear 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar.",
"1027 — Births\n\nAlbert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. ... |
1027_26474757 | What information does the article about '1027' provide on 'Asia'? | August 16 – Bagrat IV becomes king of Georgia on the death of his father, George I. Queen Dowager Mariam becomes regent for her 9-year-old son. ; This is the first year of the first rabjyung (60-year) cycle to start in the Tibetan calendar. | [
"1027\n\nYear 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar.",
"1027 — Births\n\nAlbert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. ... |
1027_26474755 | From the article on '1027', restate the 'Japan' content. | Wedding of Crown Prince Atsunaga and Imperial Princess Teishi (the wife of the crown prince died in 1025 from childbirth) 19 January: Empress Ishi give birth to Imperial Princess Shoshi 16 October: Death of Empress Dowager Kenshi - Izumi Shikibu writes a poem for her memory | [
"1027\n\nYear 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar.",
"1027 — Births\n\nAlbert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. ... |
1027_26474756 | What does the article about '1027' say regarding 'Europe'? | March 26 – Pope John XIX crowns Conrad II (the Elder) and his wife Gisela of Swabia as Holy Roman Emperor and Empress, respectively, in Old St. Peter's Basilica in Rome. Cnut the Great, King of Denmark and England, attends the coronation, proving his position as sole ruler of the Danish North Sea Empire. ; May 14... | [
"1027\n\nYear 1027 (MXXVII) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar.",
"1027 — Births\n\nAlbert III, count of Namur (House of Namur) (approximate date) ; Al-Mu'tamid ibn Abbad, Abbadid ruler of Seville (d. 1095) ; Ernest the Brave, margrave of Austria (d. ... |
1027_Aesculapia_21323239 | Describe the 'Diameter and albedo' section of the article about '1027 Aesculapia'. | According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Aesculapia measures between 31.225 and 38.55 kilometers in diameter, and its surface has an albedo between and 0.06 and 0.12... | [
"1027 Aesculapia — Diameter and albedo\n\nAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Aesculapia measures between 31.225 and 38.55 kilometers in diameter, and its s... |
1027_Aesculapia_21323238 | From the article on '1027 Aesculapia', restate the 'Classification and orbit' content. | Aesculapia is a member of the Themis family, a dynamical group of carbonaceous outer-belt asteroids which are known for their nearly coplanar ecliptical orbits. It orbits the Sun at a distance of 2.7–3.6 AU once every 5 years and 7 months (2,044 days). Its orbit has an eccentricity of 0.13 and an inclination of 1° with... | [
"1027 Aesculapia — Diameter and albedo\n\nAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Aesculapia measures between 31.225 and 38.55 kilometers in diameter, and its s... |
1027_Aesculapia_21323241 | What information does the article about '1027 Aesculapia' provide on 'Naming'? | This minor planet was named for Aesculapius, the Greek and Roman demigod of medicine and healing, son of Apollo and Coronis, after whom the asteroids 158 Koronis and 1862 Apollo are named, respectively. Naming citation was first mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 98). | [
"1027 Aesculapia — Diameter and albedo\n\nAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Aesculapia measures between 31.225 and 38.55 kilometers in diameter, and its s... |
1027_in_Norway_26496303 | Based on the article about '1027 in Norway', describe the 'Events' section. | Battle of Boknafjorden. ; The king Olaf Haraldsson had the local powerful chieftain Erling Skjalgsson killed after the Battle of Boknafjorden. After this he lost his support, fled from the country to Russia the following year, and when he returned he was defeated in the Battle of Stiklestad in 1030. | [
"1027 in Norway — Incumbents\n\nMonarchs – Olaf II",
"1027 in Norway — Events\n\nBattle of Boknafjorden. ; The king Olaf Haraldsson had the local powerful chieftain Erling Skjalgsson killed after the Battle of Boknafjorden. After this he lost his support, fled from the country to Russia the following year, ... |
1028_25112392 | Summarize the 'Births' part of '1028'. | February 17 – Al-Juwayni, Persian scholar and imam (d. 1085) ; Burchard II (or Bucco), bishop of Halberstadt (approximate date) ; Nuño Álvarez de Carazo, Spanish nobleman and warrior (d. 1054) ; Qutb Shah, Persian Sufi religious leader and scholar (d. 1099) ; Robert of Molesme, founder of the Cistercian Order (d.... | [
"1028 — Births\n\nFebruary 17 – Al-Juwayni, Persian scholar and imam (d. 1085) ; Burchard II (or Bucco), bishop of Halberstadt (approximate date) ; Nuño Álvarez de Carazo, Spanish nobleman and warrior (d. 1054) ; Qutb Shah, Persian Sufi religious leader and scholar (d. 1099) ; Robert of Molesme, founder of th... |
1028_25112389 | Describe the 'Byzantine Empire' section of the article about '1028'. | November 11 – Emperor Constantine VIII dies at Constantinople after a 3-year reign. On his deathbed, and without a male heir, Constantine arranges that his eldest daughter, Zoë Porphyrogenita, succeeds him and marries the Byzantine nobleman, Romanos III (Argyros). ; November 15 – Zoë Porphyrogenita takes th... | [
"1028 — Births\n\nFebruary 17 – Al-Juwayni, Persian scholar and imam (d. 1085) ; Burchard II (or Bucco), bishop of Halberstadt (approximate date) ; Nuño Álvarez de Carazo, Spanish nobleman and warrior (d. 1054) ; Qutb Shah, Persian Sufi religious leader and scholar (d. 1099) ; Robert of Molesme, founder of th... |
1028_25112388 | Describe the content of the article about '1028'. | Year 1028 (MXXVIII) was a leap year starting on Monday (link will display the full calendar) of the Julian calendar. | [
"1028 — Births\n\nFebruary 17 – Al-Juwayni, Persian scholar and imam (d. 1085) ; Burchard II (or Bucco), bishop of Halberstadt (approximate date) ; Nuño Álvarez de Carazo, Spanish nobleman and warrior (d. 1054) ; Qutb Shah, Persian Sufi religious leader and scholar (d. 1099) ; Robert of Molesme, founder of th... |
1028_25112391 | Reconstruct the content about 'Europe' from the article on '1028'. | April 14 – The 10-year-old Henry III (the Black), son of Emperor Conrad II (the Elder), is elected and crowned king of Germany in Aachen Cathedral by Pilgrim, archbishop of Cologne. ; King Sancho Garcés III (the Great) conquers Castile (modern Spain) (approximate date). | [
"1028 — Births\n\nFebruary 17 – Al-Juwayni, Persian scholar and imam (d. 1085) ; Burchard II (or Bucco), bishop of Halberstadt (approximate date) ; Nuño Álvarez de Carazo, Spanish nobleman and warrior (d. 1054) ; Qutb Shah, Persian Sufi religious leader and scholar (d. 1099) ; Robert of Molesme, founder of th... |
1028_Lydina_21323254 | Based on the article about '1028 Lydina', describe the 'Diameter and albedo' section. | According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lydina measures between 71.38 and 97.18 kilometers in diameter and its surface has an albedo between 0.0318 and 0.0586. The Collaborative ... | [
"1028 Lydina — Diameter and albedo\n\nAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lydina measures between 71.38 and 97.18 kilometers in diameter and its surface has an albedo bet... |
1028_Lydina_21323250 | Reconstruct the content from the article about '1028 Lydina'. | 1028 Lydina, provisional designation, is a carbonaceous background asteroid and member of the Cybele group from the outermost regions of the asteroid belt, approximately 82 km in diameter. It was discovered at the Simeiz Observatory on the Crimean peninsula on 6 November 1923, by Soviet astronomer Vladimir Albitsky, wh... | [
"1028 Lydina — Diameter and albedo\n\nAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lydina measures between 71.38 and 97.18 kilometers in diameter and its surface has an albedo bet... |
1028_Lydina_21323251 | Describe the 'Orbit and classification' section of the article about '1028 Lydina'. | Lydina is a non-family asteroid from the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. Based on osculating Keplerian orbital elements, the asteroid is considered a member of the dynamical Cybele group, which are asteroid with low orbital inclinations ... | [
"1028 Lydina — Diameter and albedo\n\nAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lydina measures between 71.38 and 97.18 kilometers in diameter and its surface has an albedo bet... |
1028_Lydina_21323255 | Summarize the 'Naming' part of '1028 Lydina'. | This minor planet was named after Lydia Il'inichna Albitskaya, wife of the discoverer Vladimir Albitsky (1891–1952). No accurate naming citation was given for this asteroid in The Names of the Minor Planets. The author of the Dictionary of Minor Planets, Lutz Schmadel, learned about the naming circumstances from Nikola... | [
"1028 Lydina — Diameter and albedo\n\nAccording to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lydina measures between 71.38 and 97.18 kilometers in diameter and its surface has an albedo bet... |
1029_26474761 | Summarize the following section from the article on '1029'. | Year 1029 (MXXIX) was a common year starting on Wednesday (link will display the full calendar) of the Julian calendar. | [
"1029\n\nYear 1029 (MXXIX) was a common year starting on Wednesday (link will display the full calendar) of the Julian calendar.",
"1029 — Births\n\nJanuary 20 – Alp Arslan (Heroic Lion), sultan of the Seljuk Empire (d. 1072) ; July 5 – Al-Mustansir Billah, caliph of the Fatimid Caliphate (d. 1094) ; ... |
1029_26474764 | What information does the article about '1029' provide on 'Births'? | January 20 – Alp Arslan (Heroic Lion), sultan of the Seljuk Empire (d. 1072) ; July 5 – Al-Mustansir Billah, caliph of the Fatimid Caliphate (d. 1094) ; Abū Ishāq Ibrāhīm al-Zarqālī, Arab astrologer and astronomer (d. 1087) ; Al-Humaydī, Andalusian scholar and writer of Islamic studies (d. 1095) ; Clement I... | [
"1029\n\nYear 1029 (MXXIX) was a common year starting on Wednesday (link will display the full calendar) of the Julian calendar.",
"1029 — Births\n\nJanuary 20 – Alp Arslan (Heroic Lion), sultan of the Seljuk Empire (d. 1072) ; July 5 – Al-Mustansir Billah, caliph of the Fatimid Caliphate (d. 1094) ; ... |
1029_26474762 | What does the article about '1029' say regarding 'Europe'? | Prince Pandulf IV of Capua becomes the de facto ruler of southern Italy – holding Capua and Naples himself – this in support with his powerful allies Amalfi, Salerno and Benevento. Only the Duchy of Gaeta remains out of his grasp. ; Rainulf Drengot, head of a mercenary band of Norman knights, is approached by Duke John... | [
"1029\n\nYear 1029 (MXXIX) was a common year starting on Wednesday (link will display the full calendar) of the Julian calendar.",
"1029 — Births\n\nJanuary 20 – Alp Arslan (Heroic Lion), sultan of the Seljuk Empire (d. 1072) ; July 5 – Al-Mustansir Billah, caliph of the Fatimid Caliphate (d. 1094) ; ... |
1029_26474765 | Summarize the 'Deaths' part of '1029'. | January 20 – Heonae, Korean queen consort and regent (b. 964) ; January 27 – Unwan (or Unwin), archbishop of Hamburg-Bremen ; May 28 – Herman of Ename, count of Verdun (Lower Lorraine) ; Abu'l-Qasim Jafar, Buyid statesman and vizier (Fasanjas family) ; Al-Karaji, Persian mathematician and engineer (ap... | [
"1029\n\nYear 1029 (MXXIX) was a common year starting on Wednesday (link will display the full calendar) of the Julian calendar.",
"1029 — Births\n\nJanuary 20 – Alp Arslan (Heroic Lion), sultan of the Seljuk Empire (d. 1072) ; July 5 – Al-Mustansir Billah, caliph of the Fatimid Caliphate (d. 1094) ; ... |
1029_La_Plata_21323307 | Reconstruct the content about 'Rotation period' from the article on '1029 La Plata'. | In October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a brightness variation of 0.58 magnitude (U... | [
"1029 La Plata — Rotation period\n\nIn October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a b... |
1029_La_Plata_21323304 | Reconstruct the content from the article about '1029 La Plata'. | 1029 La Plata, provisional designation, is a stony Koronis asteroid from the outer regions of the asteroid belt, approximately 20 km in diameter. It was discovered on 28 April 1924, by German astronomer Johannes Hartmann at the La Plata Astronomical Observatory in Argentina. It was named after the city of La Plata, Arg... | [
"1029 La Plata — Rotation period\n\nIn October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a b... |
1029_La_Plata_21323305 | What information does the article about '1029 La Plata' provide on 'Orbit and classification'? | La Plata is a member of the Koronis family (605), a prominent asteroid family with nearly co-planar ecliptical orbits and one of the largest families in the main belt at all. It orbits the Sun in the outer asteroid belt at a distance of 2.8–3.0 AU once every 4 years and 11 months (1,794 days; semi-major axis of 2.89 AU... | [
"1029 La Plata — Rotation period\n\nIn October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a b... |
1029_La_Plata_21323308 | Reconstruct the content about 'Diameter and albedo' from the article on '1029 La Plata'. | According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, La Plata measures between 16.46 and 20.78 kilometers in diameter and its surface has an albedo between 0.1819 and 0.310. The Collaborative... | [
"1029 La Plata — Rotation period\n\nIn October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a b... |
1029_La_Plata_21323309 | From the article on '1029 La Plata', restate the 'Naming' content. | This minor planet was named after the city of La Plata, Argentina, where the discovering La Plata Astronomical Observatory is located. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 98). | [
"1029 La Plata — Rotation period\n\nIn October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a b... |
1029_La_Plata_21323306 | Based on the article about '1029 La Plata', describe the 'Physical characteristics' section. | In the Tholen classification, La Plata is a common, stony S-type asteroid, which agrees with the overall spectral type for Koronian asteroids. The photometric survey conducted by Pan-STARRS also characterized it as an S-type. | [
"1029 La Plata — Rotation period\n\nIn October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a b... |
102nd_(Tyneside_Scottish)_Brigade_31331533 | Reconstruct the content about 'Active service' from the article on '102nd (Tyneside Scottish) Brigade'. | Under the command of Brigadier-General T. P. B. Ternan, the Tyneside Scottish Brigade suffered the worst losses of any brigade on 1 July 1916, the first day of the Battle of the Somme; the Tyneside Irish Brigade had the next worst tally of casualties. The 23rd (4th Tyneside Scottish) Battalion lost 629 men (19 officers... | [
"102nd (Tyneside Scottish) Brigade — Active service\n\nUnder the command of Brigadier-General T. P. B. Ternan, the Tyneside Scottish Brigade suffered the worst losses of any brigade on 1 July 1916, the first day of the Battle of the Somme; the Tyneside Irish Brigade had the next worst tally of casualties. The 23rd ... |
102nd_(Tyneside_Scottish)_Brigade_31331532 | Summarize the 'Origins' part of '102nd (Tyneside Scottish) Brigade'. | 20th Battalion, Northumberland Fusiliers (1st Tyneside Scottish) ; 21st Battalion, Northumberland Fusiliers (2nd Tyneside Scottish) ; 22nd Battalion, Northumberland Fusiliers (3rd Tyneside Scottish) ; 23rd Battalion, Northumberland Fusiliers (4th Tyneside Scottish) The Tyneside Scottish Brigade was a British First Worl... | [
"102nd (Tyneside Scottish) Brigade — Active service\n\nUnder the command of Brigadier-General T. P. B. Ternan, the Tyneside Scottish Brigade suffered the worst losses of any brigade on 1 July 1916, the first day of the Battle of the Somme; the Tyneside Irish Brigade had the next worst tally of casualties. The 23rd ... |
102nd_(Tyneside_Scottish)_Brigade_31331534 | Summarize the 'Memorial' part of '102nd (Tyneside Scottish) Brigade'. | A memorial was dedicated to the fallen of the Tyneside Scottish Brigade, at La Boiselle for their part in its capture. It was unveiled by Marshal Ferdinand Foch. | [
"102nd (Tyneside Scottish) Brigade — Active service\n\nUnder the command of Brigadier-General T. P. B. Ternan, the Tyneside Scottish Brigade suffered the worst losses of any brigade on 1 July 1916, the first day of the Battle of the Somme; the Tyneside Irish Brigade had the next worst tally of casualties. The 23rd ... |
102nd_Battalion,_CEF_6958965 | Summarize the following section from the article on '102nd Battalion, CEF'. | Lt.-Col. John Weightman Warden, DSO, 18 June 1916 – 11 January 1918 ; Lt.-Col. F. Lister, CMG, DSO, MC, 11 January 1918 – 27 September 1918 ; Lt.-Col. E.J.W. Ryan, DSO, 28 September 1918 – 19 November 1918 ; Lt.-Col. F. Lister, CMG, DSO, MC, 19 November 1918-Demobilization , 1 July–18 November 1916 ; Ancre Heights, 1 O... | [
"102nd Battalion, CEF — Sources\n\nCanadian Expeditionary Force 1914–1919 by Col. G.W.L. Nicholson, CD, Queen's Printer, Ottawa, Ontario, 1962",
"102nd Battalion, CEF\n\nLt.-Col. John Weightman Warden, DSO, 18 June 1916 – 11 January 1918 ; Lt.-Col. F. Lister, CMG, DSO, MC, 11 January 1918 – 27 September 1918 ; Lt... |
102nd_Battalion,_CEF_6958966 | Summarize the following section from the article on '102nd Battalion, CEF'. | du Nord, 27 September–2 October 1918 Canal du Nord, 27 September–2 October 1918 The 102nd Battalion, CEF, (initially the 102nd Battalion (Northern British Columbia), then after August, 1917, the 102nd Battalion (Central Ontario), CEF) was an infantry battalion of the Great War Canadian Expeditionary Force. The 102nd Ba... | [
"102nd Battalion, CEF — Sources\n\nCanadian Expeditionary Force 1914–1919 by Col. G.W.L. Nicholson, CD, Queen's Printer, Ottawa, Ontario, 1962",
"102nd Battalion, CEF\n\nLt.-Col. John Weightman Warden, DSO, 18 June 1916 – 11 January 1918 ; Lt.-Col. F. Lister, CMG, DSO, MC, 11 January 1918 – 27 September 1918 ; Lt... |
102nd_Battalion,_CEF_6958967 | Reconstruct the content from the article about '102nd Battalion, CEF'. | at Comox, on Vancouver Island. During the attack on Vimy Ridge, the 102nd lost most of its officers and for a time was led by one of the company sergeant-majors. The battalion achieved its objectives for the day but lost 314 killed or wounded. The 102nd Battalion had four Officers Commanding: One member of the 102nd Ba... | [
"102nd Battalion, CEF — Sources\n\nCanadian Expeditionary Force 1914–1919 by Col. G.W.L. Nicholson, CD, Queen's Printer, Ottawa, Ontario, 1962",
"102nd Battalion, CEF\n\nLt.-Col. John Weightman Warden, DSO, 18 June 1916 – 11 January 1918 ; Lt.-Col. F. Lister, CMG, DSO, MC, 11 January 1918 – 27 September 1918 ; Lt... |
102nd_Cavalry_Regiment_20229289 | What information does the article about '102nd Cavalry Regiment' provide on 'ANNEX 5'? | Constituted 9 July 1946 in the New Jersey National Guard as the 113th Tank Battalion and assigned to the 50th Armored Division Organized and federally recognized 8 April 1947 in eastern New Jersey with headquarters at Orange (Location of headquarters changed 31 December 1947 to Dover) Redesignated 1 March 1949 as the 1... | [
"102nd Cavalry Regiment — ANNEX 5\n\nConstituted 9 July 1946 in the New Jersey National Guard as the 113th Tank Battalion and assigned to the 50th Armored Division Organized and federally recognized 8 April 1947 in eastern New Jersey with headquarters at Orange (Location of headquarters changed 31 December 1947 to ... |
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