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HD 3240 [SEP] constellation | HD 3240
HD 3240 is a 5th magnitude star in the constellation Cassiopeia, approximately 540 light years away from Earth. It is a bluish white giant star of the spectral type B7III, meaning its surface temperature is at least twice as hot as that of the Sun, and it is many times larger and brighter. | ' have Intel HD Graphics 4000; others have Intel HD Graphics 2500
- All variants have GPU base frequencies of 650 MHz and peak GPU turbo frequencies of 1.05 GHz
- TDP 55 W
- Variants
- i3-3220T – 2.8 GHz
- i3-3240T – 2.9 GHz
- i3-3210 – 3.2 GHz
- i3-3220 – 3.3 GHz
- i3-3225 – 3.3 GHz
- i3-3240 – 3.4 GHz | 11,000 | zeroshot-train |
HD 38283 [SEP] constellation | HD 38283
HD 38283 is a 7th magnitude F-type main sequence star located approximately 125 light-years away in the constellation of Mensa. HD 38283 is not visible to the naked eyes for most people but can be easily seen using binoculars.
Planetary system.
On April 11, 2011, a Saturnian planet, HD 38283 b, was discovered ... | similar distance from its parent star as Earth. But, given the planet's high eccentricity, and the star being more than twice as luminous as our Sun, hypothetical life on the moons may be a bit unlikely.
HD 38283 b was discovered on 11 April 2011 using the radial velocity technique using the Anglo-Australian Telescope ... | 11,001 | zeroshot-train |
HD 41742/41700 [SEP] constellation | HD 41742/41700
HD 41742/41700 is a star system that lies approximately 87 light-years away in the constellation of Puppis. The system consists of two bright stars where the primary is orbited by two fainter stars, making it a quadruple with an unequal hierarchy.
Component discovery.
HD 41742 B was discovered early on i... | , HD 41700 has a somewhat large lithium content; because lithium is used up by a star at an approximately constant rate over its lifetime, this can be used to estimate a star's age. For HD 41700, its lithium abundance indicates an age of 200 ± 50 million years.
Some young star systems remain loosely associated with oth... | 11,002 | zeroshot-train |
HD 47186 [SEP] constellation | HD 47186
HD 47186 is a star located approximately 129 light-years away in the constellation of Canis Major. It is a G6V star with the characteristics very similar to the Sun, but it is 1.7 times more metal-rich. In 2008, two extrasolar planets were discovered orbiting the star.
Planetary system.
Announced in June 2008,... | the Solar System in a few billion years as the Sun ages and becomes a giant. Conversely, HD 45364 is a star 107 light-years distant that is a little smaller and cooler than the Sun, of spectral type G8V, which has two planets discovered in 2008. With orbital periods of 228 and 342 days, the planets have a 3:2 orbital r... | 11,003 | zeroshot-train |
HD 48265 [SEP] constellation | HD 48265
HD 48265 is the Henry Draper Catalogue designation for a star in the southern constellation Puppis. It has an apparent visual magnitude of 8.07, which makes it too faint to be seen with the naked eye. Based upon parallax measurements made during the Hipparcos mission, it is located at a distance of roughly fro... | HD 145377 b
HD 145377 b is an extrasolar planet located approximately 180 light-years awayThis planet was discovered on October 26, 2008 by Moutou "et al." using the HARPS spectrograph on ESO's 3.6 meter telescope installed at La Silla Observatory in Atacama desert, Chile.
See also.
- BD-17°63 b
- HD 131664
- HD 143361... | 11,004 | zeroshot-train |
HD 53143 [SEP] constellation | HD 53143
HD 53143 is a star in the Carina constellation, located about from the Earth. With an apparent visual magnitude of 6.80, this star is a challenge to view with the naked eye even under ideal viewing conditions.
Using the technique of gyrochronology, which measures the age of a low-mass star based on its rotatio... | (2009)
External links.
- The Circumstellar Disk Learning Site
- Kalas' homepage
- Sky & Telescope Article on Fomalhaut discovery
- Space.com article on AU Microscopii discovery
- New Scientist article on HD 53143 and HD 139664 discoveries | 11,005 | zeroshot-train |
HD 6434 [SEP] constellation | HD 6434
HD 6434 is an 8th magnitude star in the constellation of Phoenix. It is a very Sun-like yellow dwarf star, but much older, being 12.2 billion years old. Yellow dwarfs are not very luminous, so at a distance of 138 light years it is not visible to the unaided eye. With binoculars it is readily visible under idea... | HD 6434 b
HD 6434 b is an extrasolar planet orbiting the star HD 6434. It has a minimum mass about half that of Jupiter. It orbits the star very close, over 2.5 times as close as Mercury orbits the Sun. For this reason it completes one orbit in only 22 days. Unlike true "hot Jupiters" like 51 Pegasi b, HD 6434 b does n... | 11,006 | zeroshot-train |
HD 69830 [SEP] constellation | HD 69830
HD 69830 (285 G. Puppis) is a yellow dwarf star located approximately 41 light-years away in the constellation of Puppis. In 2005, the Spitzer Space Telescope discovered a narrow ring of warm debris orbiting the star. The debris ring contains substantially more dust than the Solar System's asteroid belt. In 20... | HD 23079 b
HD 23079 b is an exoplanet approximately 109 light years away in the constellation Reticulum. The planet has mass of at least 2.45 Jupiters, although only the minimum mass is known since inclination is unknown. The planet takes almost exactly two years to orbit the star at the average distance of 1.6 AU. The... | 11,007 | zeroshot-train |
HD 82785 [SEP] constellation | HD 82785
HD 82785 is star in the southern constellation of Antlia.
External links.
- Image HD 82785 | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,008 | zeroshot-train |
HD 88809 [SEP] constellation | HD 88809
HD 88809 is a star in a double star system in the constellation Antlia. The primary is an orange giant of spectral type K1III. Located around 480 light-years distant, it shines with a luminosity approximately 124 times that of the Sun and has a surface temperature of 4607 K. It has an apparent magnitude of 5.9... | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,009 | zeroshot-train |
HD 89307 b [SEP] constellation | HD 89307 b
HD 89307 b is an extrasolar planet orbiting the star HD 89307 located approximately 108 light-years away in the constellation of Leo. The planet takes 187 megaseconds to orbit (roughly 2164 days or 5.9 years). The planet's minimum mass is 1.92 M since the inclination is unknown. As it is typical for most of ... | HD 7924 b
HD 7924 b is an extrasolar planet located approximately 55 light years away in the constellation of Cassiopeia, orbiting the 7th magnitude K-type main sequence (slightly metal poor) star HD 7924. It was published on January 28, 2009 and is the second planet discovered in the constellation Cassiopeia. Two addi... | 11,010 | zeroshot-train |
HIP 12961 [SEP] constellation | HIP 12961
HIP 12961 is a dim red dwarf star located approximately 75 light-years away in the constellation of Eridanus. It is one of the largest and brightest M class red dwarf stars known. In 2009 an extrasolar planet orbiting this faint star has been announced.
Planetary system.
HIP 12961 b is an extrasolar planet wh... | are very-low-mass stars. As a result, they have relatively low pressures, a low fusion rate, and hence, a low temperature. The energy generated is the product of nuclear fusion of hydrogen into helium by way of the proton–proton (PP) chain mechanism. Hence, these stars emit little light, sometimes as little as that of ... | 11,011 | zeroshot-train |
HR 2554 [SEP] constellation | HR 2554
HR 2554, also known as V415 Carinae and A Carinae, is an eclipsing spectroscopic binary of the Algol type in the constellation of Carina whose apparent visual magnitude varies by 0.06 magnitudes and is approximately 4.39 at maximum brightness. Its primary is a G-type bright giant star and its secondary is an A-... | versions of the same bill, the "MLK Records Act" (one in 2003, the other in 2005), which, if signed into law, would release all currently sealed files concerning the 1968 assassination of Martin Luther King Jr. These records were sealed in 1978 and are not due to be declassified until the year 2028. The 2005 version of... | 11,012 | zeroshot-train |
IC 10 [SEP] constellation | IC 10
IC 10 is an irregular galaxy in the constellation Cassiopeia. It was discovered by Lewis Swift in 1887 and in 1935 Nicholas Mayall became the first to suggest that the object is extragalactic. Edwin Hubble suspected it might belong to the Local Group of galaxies, but its status remained uncertain for decades. The... | NGC 3464
NGC 3464 is a barred spiral galaxy in the constellation of Hydra, discovered 14 January 1886 by Ormond Stone.
Supernovae.
Two supernovae were observed in NGC 3464 in 2002. SN 2002J, a Type Ic supernova, was detected 21 January, and SN 2002hy, a Type Ib supernova, was detected 12 November. A Type Ia supernova, ... | 11,013 | zeroshot-train |
KELT-2A [SEP] constellation | KELT-2A
KELT-2A (HD 42176A) is a yellow white dwarf star located about 440 light-years away in the constellation Auriga. The apparent magnitude of this star is 8.77, which means it is not visible to the naked eye but can be seen with a binoculars.
KELT-2A is the brightest star in the common-proper-motion binary star sy... | KELT-2A is a member of the common-proper-motion binary star system KELT-2 (HD 42176). KELT-2B is an early K dwarf approximately 295 astronomical units away.
See also.
- KELT
External links.
- KELT-North survey website
- KELT-2Ab discovery lightcurve, with music | 11,014 | zeroshot-train |
KELT-2Ab [SEP] constellation | KELT-2Ab
KELT-2Ab is an extrasolar planet that orbits the star KELT-2A approximately 440 light-years away in the constellation of Auriga. It was discovered by the KELT-North survey via the transit method, so both its mass and radius are known quite precisely. As of its discovery KELT-2Ab is the fifth-brightest transiti... | system found so far researchers expect it may be useful in learning more about inflated planets.
Star system.
KELT-4 is a triple star system. KELT-4BC is a binary star system subcomponent of the triple, away from KELT-4A and the projected separation between KELT-4B and KELT-4C is .
See also.
- Gliese 667 Cc, a planet i... | 11,015 | zeroshot-train |
KT Eridani [SEP] constellation | KT Eridani
KT Eridani was a bright nova, which produced an outburst in 2009 in the constellation Eridanus. It was discovered on 2009 November 25 by K. Itagaki at Yamagata, Japan. It was first called Nova Eridani 2009 and is located at . In the most common nova systems, the white dwarf accretes matter from a main sequen... | (Impact Assessment & Rehabilitation) in the Narmada Control Authority.
Ahmad has also worked for the G. B. Pant Institute of Himalayan Environment and Development, Ministry of Environment and Forests (India).
Personal life.
Afroz Ahmad married Begum Sadiya Yasmin(Afroz), daughter of poet and Politician Bekal Utsahi. Sa... | 11,016 | zeroshot-train |
Kappa Volantis [SEP] constellation | Kappa Volantis
Kappa Volantis (κ Vol, κ Volantis) is a triple star system in the constellation Volans. The primary component has an apparent visual magnitude of 5.37, while the secondary companion is magnitude 5.65. based upon parallax measurements, the stars appear to be around 420−430 light years. from the Sun.
The b... | at the Library of Congress. Enescu's letter crossed in the post with an acknowledgment of the manuscript's safe arrival, written on 17 June 1953 by Edward N. Waters, Assistant Chief of the Music Division . This autograph score contains a number of further small adjustments which may have been made as late as the spring... | 11,017 | zeroshot-train |
Kepler-11f [SEP] constellation | name "Kepler" is derived from the Kepler satellite, a NASA Earth-trailing spacecraft that constantly observes a small patch of sky between the constellations Cygnus and Lyra for stars that are transited by, in particular, terrestrial planets. As these planets cross in front of their host stars with respect to Earth, a ... | Kepler-11f
Kepler-11f is an exoplanet (extrasolar planet) discovered in the orbit of the sun-like star Kepler-11 by NASA's Kepler spacecraft, which searches for planets that transit (cross in front of) their host stars. Kepler-11f is the fifth planet from its star, orbiting one quarter of the distance (.25 AU) of the E... | 11,018 | zeroshot-train |
Kepler-23c [SEP] constellation | Kepler-23c
Kepler-23c is a Neptune-sized exoplanet orbiting the star Kepler-23, located in the constellation Cygnus. The planet is 3.12 times wider than the Earth and is 0.189 Jupiter masses. The planet was discovered using data taken from "Kepler" spacecraft. It is likely a gas giant. | Kepler-9b
Kepler-9b is one of the first planets discovered outside the solar system (exoplanets) by NASA's Kepler Mission. It revolves around the star Kepler-9 within the constellation Lyra. Kepler-9b is the largest of three planets detected in the Kepler system by transit method; its mass is roughly half that of the p... | 11,019 | zeroshot-train |
Kepler-42 [SEP] constellation | Kepler-42
Kepler-42, formerly known as KOI-961, is a red dwarf located in the constellation Cygnus and approximately 131 light years from the Sun. It has three known extrasolar planets, all of which are smaller than Earth in radius, and likely also in mass.
Characteristics.
Kepler-42's mass is estimated to be 0.13 time... | Kepler-9b
Kepler-9b is one of the first planets discovered outside the solar system (exoplanets) by NASA's Kepler Mission. It revolves around the star Kepler-9 within the constellation Lyra. Kepler-9b is the largest of three planets detected in the Kepler system by transit method; its mass is roughly half that of the p... | 11,020 | zeroshot-train |
Medusa Nebula [SEP] constellation | Medusa Nebula
The Medusa Nebula is a large planetary nebula in the constellation of Gemini on the Canis Minor border. It is also known as Abell 21 and Sharpless 2-274. It was originally discovered in 1955 by UCLA astronomer George O. Abell, who classified it as an old planetary nebula. The braided serpentine filaments ... | - The Hercules Cluster is a group of stars observed in "The Wheel in Space".
- Kasterborous is the constellation in which Gallifrey is located.
- The Lotus Nebula is mentioned by John Hart as being where he could be experiencing 17 simultaneous pleasures in the episode "Exit Wounds".
- The Medusa Cascade is an Interuni... | 11,021 | zeroshot-train |
Messier 3 [SEP] constellation | Messier 3
Messier 3 (M3 or NGC 5272) is a globular cluster of stars in the northern constellation of Canes Venatici. It was discovered on May 3, 1764, and was the first Messier object to be discovered by Charles Messier himself. Messier originally mistook the object for a nebula without stars. This mistake was correcte... | Messier 9
Messier 9 or M9 (also designated NGC 6333) is a globular cluster in the constellation of Ophiuchus. It is positioned in the southern part of the constellation to the southwest of Eta Ophiuchi, and lies atop a dark cloud of dust designated Barnard 64. The cluster was discovered by French astronomer Charles Mes... | 11,022 | zeroshot-train |
Messier 46 [SEP] constellation | Messier 46
Messier 46 or M46, also known as NGC 2437, is an open cluster of stars in the constellation of Puppis. It was discovered by Charles Messier in 1771. Dreyer described it as "very bright, very rich, very large." M46 is about 4,920 light-years away. There are an estimated 500 stars in the cluster with a combine... | Eagle Nebula
The Eagle Nebula (catalogued as Messier 16 or M16, and as NGC 6611, and also known as the Star Queen Nebula and The Spire) is a young open cluster of stars in the constellation Serpens, discovered by Jean-Philippe de Chéseaux in 1745–46. Both the "Eagle" and the "Star Queen" refer to visual impressions of ... | 11,023 | zeroshot-train |
Messier 49 [SEP] constellation | Messier 49
Messier 49 (also known as M 49 or NGC 4472) is an elliptical galaxy located about away in the equatorial constellation of Virgo. This galaxy was discovered by French astronomer Charles Messier on February 16, 1777.
As an elliptical galaxy, Messier 49 has the physical form of a radio galaxy, but it only has ... | ) within its borders 5° to 12° west of ε Vir (Vindemiatrix), this constellation is especially rich in galaxies.
Some examples are Messier 49 (elliptical), Messier 58 (spiral), Messier 59 (elliptical), Messier 60 (elliptical), Messier 61 (spiral), Messier 84 (lenticular), Messier 86 (lenticular), Messier 87 (elliptical ... | 11,024 | zeroshot-train |
NGC 1300 [SEP] constellation | NGC 1300
NGC 1300 is a barred spiral galaxy located about 61 million light-years away in the constellation Eridanus. The galaxy is about 110,000 light-years across (about the same size of the Milky Way). It is a member of the Eridanus Cluster, a cluster of 200 galaxies. It was discovered by John Herschel in 1835.
In th... | NGC 3054
NGC 3054 is an intermediate spiral galaxy in the constellation Hydra. It was discovered by Christian Heinrich Friedrich Peters in 1859. It is probably in the same galaxy group as NGC 2935.
In January 2006, a supernova (SN 2006T) was observed in NGC 3054.
See also.
- New General Catalogue (NGC)
- NGC 1300
Ext... | 11,025 | zeroshot-train |
NGC 1555 [SEP] constellation | NGC 1555
NGC 1555, sometimes known as Hind's Variable Nebula, is a variable nebula, illuminated by the star T Tauri, located in the constellation Taurus. It is also in the second Sharpless catalog as 238. It is a Herbig–Haro object. The nebula was discovered on October 11, 1852 by John Russell Hind.
See also.
- NGC 226... | NGC 6520
NGC 6520 is an open cluster in the constellation Sagittarius. It is magnitude 9.0, diameter 5 arc minutes and class G. It has about 25 stars of magnitude 9 to 12. A dark nebula B86 near its western edge.
References.
- Robert Burnham, Jr, "Burnham's Celestial Handbook: An observer's guide to the universe beyond... | 11,026 | zeroshot-train |
NGC 2241 [SEP] constellation | NGC 2241
NGC 2241 is an open cluster in the constellation Dorado. Located in the Large Magellanic Cloud, it was discovered by John Herschel on January 31, 1835.
External links.
- NED – NGC 2241
- SEDS – NGC 2241
- VizieR – NGC 2241 | all European official languages and export it into the following formats: PDF, ODT, HTML, XHTML, HR-XML. The plugin is compliant with HR-XML SEP specifications. Last version of the plugin has been released in January 2008.
History.
The Europass framework was established by Decision 2241/2004/EC of the European Parliame... | 11,027 | zeroshot-train |
NGC 2546 [SEP] constellation | NGC 2546
NGC 2546 is an open cluster in the constellation Puppis, discovered by Abbe Lacaille in 1751-1752 from South Africa. | 25
First Partial Lunar Eclipse: 2041 May 16
First Total Lunar Eclipse: 2167 Aug 01
First Central Lunar Eclipse: 2221 Sep 02
Greatest Eclipse of the Lunar Saros 141: 2293 Oct 16
Last Central Lunar Eclipse: 2546 Mar 18
Last Total Lunar Eclipse: 2618 May 01
Last Partial Lunar Eclipse: 2744 Jul 16
Last Penumbral Lunar Ecli... | 11,028 | zeroshot-train |
NGC 28 [SEP] constellation | NGC 28
NGC 28 is an elliptical galaxy located in the Phoenix constellation. It was discovered on the 28th October 1834 by John Herschel.
NGC 28 2MASS (near-infrared) | NGC 217
NGC 217 is a spiral or lenticular galaxy located approximately 178 light-years from the Solar System in the constellation Cetus. It was discovered on November 28, 1785 by William Herschel.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Cetus (constellation)
External links.
- | 11,029 | zeroshot-train |
NGC 2808 [SEP] constellation | NGC 2808
NGC 2808 is a globular cluster in the constellation Carina. The cluster belongs to the Milky Way, and is one of our home galaxy's most massive clusters, containing more than a million stars. It is estimated to be 12.5-billion years old.
Star Generations.
It had been thought that NGC 2808, like typical globular... | Hubble Space Telescope images of NGC 2808 taken in 2005 and 2006 with Hubble's Advanced Camera for Surveys. Unexpectedly, they found that this cluster is composed of three generations of stars, all born within 200 million years of the formation of the cluster.
Astronomers have argued that globular clusters can produce ... | 11,030 | zeroshot-train |
NGC 2903 [SEP] constellation | NGC 2903
NGC 2903 is a field barred spiral galaxy about 30 million light-years away in the constellation Leo. It was discovered by William Herschel who cataloged it on November 16, 1784. NGC 2903 has a very high rate of star formation in its central region. NGC 2905 is a bright star cloud within this galaxy.
NGC 2903 ... | five galactic star forming regions have associated formaldehyde maser emission, which has only been observed through the 1 → 1 transition. Because of the widespread interest in interstellar formaldehyde it has recently been extensively studied, yielding new extragalactic sources, including NGC 253, NGC 520, NGC 660, NG... | 11,031 | zeroshot-train |
NGC 3242 [SEP] constellation | NGC 3242
NGC 3242, commonly known as the Ghost of Jupiter, is a planetary nebula located in the constellation Hydra.
William Herschel discovered the nebula on February 7, 1785, and cataloged it as H IV.27. John Herschel observed it from the Cape of Good Hope, South Africa, in the 1830s, and numbered it as h 3248, and i... | in false-color pictures. NGC 3242 can easily be observed with amateur telescopes and appears bluish-green to most observers. Larger telescopes can distinguish the outer halo as well.
See also.
- List of NGC objects
- Planetary nebulae
External links.
- The Hubble European Space Agency Information Centre – Hubble pictur... | 11,032 | zeroshot-train |
NGC 3271 [SEP] constellation | NGC 3271
NGC 3271 is a barred spiral galaxy in the constellation Antlia. At magnitude 11.7, it is the brightest spiral galaxy in the Antlia Cluster, which lies about away. | , N. Yudanin, M. I. Muller, I. Davis, D. Farber, P. Hartjen, F. Haag, G. Alter, J. Schulze zur Wiesch, H. Streeck: "Expansion of HIV-specific T follicular helper cells in chronic HIV infection" In: "Journal of Clinical Investigation." 122(9), 4. Sep 2012, S. 3271–3280.
- M. F. Chevalier, B. Jülg, A. Pyo, M. Flanders, S... | 11,033 | zeroshot-train |
NGC 3842 [SEP] constellation | NGC 3842
NGC 3842 is an elliptical galaxy in the constellation of Leo. It was discovered by William Herschel. It is notable for containing one of the largest black holes ever detected, reported to have a mass of 9.7 billion solar masses. It is around 330 million light-years distant from Earth.
NGC 3842 is the brightest... | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,034 | zeroshot-train |
NGC 4485 [SEP] constellation | NGC 4485
NGC 4485 is an irregular galaxy located in the constellation of Canes Venatici. It is interacting with the spiral galaxy NGC 4490 and as a result both galaxies are distorted and are undergoing intense star formation. | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,035 | zeroshot-train |
NGC 4639 [SEP] constellation | NGC 4639
NGC 4639 is a barred spiral galaxy located in the constellation Virgo. It lies over 70 million light-years away from planet Earth. Its core contains a massive black hole. NGC 4639 is also classified as a Seyfert galaxy. NGC 4639 is a member of the Virgo Cluster. | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,036 | zeroshot-train |
NGC 474 [SEP] constellation | NGC 474
NGC 474 is an elliptical galaxy about 100 million light years distant in the constellation Pisces. This large galaxy is known to possess tidal tails, although their origins remain unknown.
Supernova.
In July 2017 a Type Ia supernova designated SN 2017fgc was discovered in NGC 474. It was located a considerable ... | NGC 7600
NGC 7600 is an elliptical galaxy about 160 million light-years in the constellation Aquarius classified as a lenticular galaxy, or, more formally, an S0 galaxy.
External links.
- Preprint version of 1999MNRAS.307..967T with images of shell galaxies NGC 474 and NGC 7600
- The formation of shell galaxies similar... | 11,037 | zeroshot-train |
NGC 5164 [SEP] constellation | NGC 5164
NGC 5164 is a galaxy in the constellation Ursa Major. It was discovered by William Herschel on April 14, 1789. | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,038 | zeroshot-train |
NGC 5334 [SEP] constellation | NGC 5334
NGC 5334 is a face-on spiral galaxy in the constellation Virgo.
External links.
- NASA/IPAC Extragalactic Database: Pictures and description | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,039 | zeroshot-train |
NGC 5408 [SEP] constellation | NGC 5408
NGC 5408 is an irregular galaxy in the constellation Centaurus. It was discovered by John Herschel on June 5, 1834.
Galaxy group information.
NGC 5408 is located near the M83 Subgroup of the Centaurus A/M83 Group, a relatively nearby group of galaxies. However, it is unclear as to whether NGC 5408 is part of t... | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,040 | zeroshot-train |
NGC 55 [SEP] constellation | NGC 55
NGC 55, also occasionally referred to as The Whale Galaxy, is a Magellanic type barred spiral galaxy located about 7 million light-years away in the constellation Sculptor. Along with its neighbor NGC 300, it is one of the closest galaxies to the Local Group, probably lying between the Milky Way and the Sculptor... | NGC 1073
NGC 1073 is a barred spiral galaxy in the constellation Cetus. It probably has an H II nucleus.
NGC 1073 is about 55 million light years from Earth. NGC 1073 is about 80,000 light years across. NGC 1073 can be viewed with a mid-sized telescope and is found in the Cetus constellation, also called the Sea Monste... | 11,041 | zeroshot-train |
NGC 5548 [SEP] constellation | NGC 5548
NGC 5548 is a Type I Seyfert galaxy with a bright, active nucleus. This activity is caused by matter flowing onto a 65 million solar mass () supermassive black hole at the core. Morphologically, this is an unbarred lenticular galaxy with tightly-wound spiral arms, while shell and tidal tail features suggest th... | seen in infrared.
- NGC 4945, a galaxy relatively close to Centaurus A.
- NGC 5033, has a Seyfert nucleus displaced from its kinematic center.
- NGC 5548, an example of a lenticular Seyfert galaxy
- NGC 6240, also classified as an ultraluminous infrared galaxy (ULIRG)
- NGC 6251, the X-ray brightest low-excitation radi... | 11,042 | zeroshot-train |
NGC 5820 [SEP] constellation | NGC 5820
NGC 5820 is a lenticular galaxy in the constellation Boötes. It lies near NGC 5821, a galaxy with a similar mass at the same redshift.
External links.
- Distance
- Image NGC 5820
- SIMBAD data | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,043 | zeroshot-train |
NGC 6085 [SEP] constellation | NGC 6085
NGC 6085 is a spiral galaxy in the constellation of Corona Borealis. It is classified as a LINER galaxy and is a member of Abell 2162. | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,044 | zeroshot-train |
NGC 6210 [SEP] constellation | NGC 6210
NGC 6210 is a planetary nebula located in the constellation Hercules.
See also.
- List of NGC objects
External links.
- HubbleSite NewsCenter Hubble picture and information on NGC 6210 | : "Machtpolitik" or Accommodation?". "Church History", Vol. 49, No. 3 (Sep., 1980), pp. 298–315.
- Beckman, Joachim, (ed.). Published in "Kirchliches Jahrbuch für die Evangelische Kirche in Deutschland"; vol. 60-71 (1933-1944), Joachim Beckmann (ed.) on behalf of the Evangelische Kirche in Deutschland, Gütersloh: Berte... | 11,045 | zeroshot-train |
NGC 6334 [SEP] constellation | NGC 6334
NGC 6334 (also known as the Cat's Paw Nebula, Bear Claw Nebula, or Gum 64) is an emission nebula and star-forming region located in the constellation Scorpius. It was discovered by astronomer John Herschel in 1837, who observed it from the Cape of Good Hope in South Africa.
External links.
- On the Trail of a ... | discovery in 1860 when Arthur von Auwers discovered the nova T Scorpii.
NGC 6302, also called the Bug Nebula, is a bipolar planetary nebula. NGC 6334, also known as the Cat's Paw Nebula, is an emission nebula and star-forming region.
Mythology.
In Greek mythology, the myths associated with Scorpio almost invariably als... | 11,046 | zeroshot-train |
NO Apodis [SEP] constellation | NO Apodis
NO Apodis (HD 156513) is semi-regular pulsating star located in the far southern constellation Apus. It varies between magnitudes 5.71 and 5.95, its pulsations of periods 26.2 and 26.6 days respectively. Located around 780 ± 20 light-years distant, it shines with a luminosity approximately 2059 times that of ... | the transmission to pull the tank over bumps.
In terms of performance the GT 101 would have been surprisingly effective. It would have produced a total of 3,750 hp, using 2,600 hp to operate the compressor and thus leaving 1,150 hp to power the transmission. The entire engine assembly weighed 450 kg (992 lb), not inclu... | 11,047 | zeroshot-train |
Nu Tauri [SEP] constellation | Nu Tauri
Nu Tauri (ν Tau, ν Tauri) is a star in the constellation Taurus. Nu Tauri is a white A-type main sequence dwarf with an apparent magnitude of +3.91. It is approximately 117 light years from Earth. This star is 2.2 times the mass of the Sun, more than double the Sun's radius, and is radiating roughly 34 times t... | Arrington "Early B" Neil – backing vocals
- Kay Cee – scratches, producer , arranger, mixing
- Big Snow – producer
- Robert Power – mixing
- Loren Wilson Hill – re-mixing
- Wendell "The Grinch" Hanes – re-mixing
- Tyrone "Fly Ty" Williams – executive producer
- Leonard Fichtelberg – executive producer | 11,048 | zeroshot-train |
OGLE-TR-56 [SEP] constellation | OGLE-TR-56
OGLE-TR-56 is a dim, distant, magnitude 17 Sun-like star located approximately 1500 parsecs away in the constellation of Sagittarius.
This star is listed as an eclipsing type variable star with the eclipse due to the passage of the planet as noted in the discovery papers.
Planetary system.
In 2002, a possibl... | OGLE-TR-211
OGLE-TR-211 is a distant magnitude 14 star located about 5,700 light years away in the constellation of Carina.
Planetary system.
OGLE-TR-211 has a transiting planet in a very close orbit, another hot Jupiter.
See also.
- OGLE-TR-182
- List of extrasolar planets | 11,049 | zeroshot-train |
Omega Centauri [SEP] constellation | Omega Centauri
Omega Centauri (ω Cen or NGC 5139) is a globular cluster in the constellation of Centaurus that was first identified as a non-stellar object by Edmond Halley in 1677. Located at a distance of 15,800 light-years (4,850 pc), it is the largest globular cluster in the Milky Way at a diameter of roughly 150 l... | Omega Centauri: Former Core of a Dwarf Galaxy?
- Omega Centauri: Proud Cluster or Sad Remnant?
- Omega Centauri at ESA/Hubble
- Omega Centauri on Wikisky.org
- Omega Centauri, Galactic Globular Clusters Database page
- Omega Centauri at Constellation Guide | 11,050 | zeroshot-train |
Omicron Tauri [SEP] constellation | Omicron Tauri
Omicron Tauri (ο Tau, ο Tauri) is a star in the constellation Taurus. Omicron Tauri is a yellow G-type giant with an apparent magnitude of +3.61. This star has three times the mass of the Sun and fifteen to eighteen times the Sun's radius. Based on the latter, interferometry-measured radius, it is rotatin... | Fiji.
- Laufafaetoga went to Samoa and became pregnant to Tupaimatuna. They sailed for Tonga but were blown off course and landed in Fiji. Their child was born and given the name Vaasilifiti. At this time, Fiji was in continual warfare and Lautala was the most famous warrior. Laufafaetoga and Lautala had three children... | 11,051 | zeroshot-train |
PGC 39058 [SEP] constellation | PGC 39058
PGC 39058 is a dwarf galaxy located 14 million light-years away in the constellation Draco. The galaxy is faint and obscured by HD 106381, a star in the foreground making it difficult to observe. | major and minor axis,
- 67,116 apparent magnitudes,
- 20,046 radial velocities and
- 24,361 position angles.
The Lyon-Meudon Extragalactic Database was eventually expanded into HyperLEDA, a database of a few million galaxies. Galaxies in the original PGC catalogue are numbered with their original PGC number in HyperLED... | 11,052 | zeroshot-train |
Pegasids [SEP] constellation | Pegasids
The meteor shower of the Pegasids occurs between the 7 and 13 July. It is a weak meteor shower that has its maximum around July 9 having a ZHR of only 3 meteors per hour. The meteors have, however, an atmosphere entry speed of about 70 km/s.
The Radiant of the Pegasids is in the constellation of Pegasus, aroun... | 66, 122, 131, 168, 170, 173, 234, 282.
- Dunne, Aidan. 2008. Rare encounter with sculpture in the spotlight. Irish Times, 6 Feb.
- Kenny, Padraig. 2008. The French Connection. Sunday Tribune, 28 Sep p3.
- Dunne, Aidan, 2005. The Art of Geometry. Irish Times, 23 May, p. 10.
- Woods, Suzanne and Marshall, Catherine. 2005... | 11,053 | zeroshot-train |
Phi Capricorni [SEP] constellation | Phi Capricorni
Phi Capricorni (φ Cap, φ Capricorni) is a solitary star in the southern constellation of Capricornus. It is visible to the naked eye with an apparent visual magnitude of +5.16. Based upon an annual parallax shift of 5.07 mas as seen from the Earth, the star is located about 640 light years from the Sun, ... | Ramparts", refers to an asterism consisting of Gamma Capricorni, Kappa Capricorni, Epsilon Capricorni, Delta Capricorni, Iota Aquarii, Sigma Aquarii, Lambda Aquarii, Phi Aquarii, 27 Piscium, 29 Piscium, 33 Piscium and 30 Piscium. Consequently, the Chinese name for Gamma Capricorni itself is (, ).
Nomenclature Namesake.... | 11,054 | zeroshot-train |
Psi Cygni [SEP] constellation | Psi Cygni
ψ Cygni, Latinised as Psi Cygni, is a triple star system in the constellation called Cygnus. With a combined apparent visual magnitude of 4.92, it is visible to the naked eye. As of 2002, the inner pair, components Aa and Ab, had an angular separation of 0.10 arc seconds along a position angle of 77.6°. Their... | the WGSN says that the name should be understood to be attributed to the brightest component by visual brightness - in this case Pi¹ Cygni A.
In Chinese, (), meaning "Flying Serpent", refers to an asterism consisting of Pi¹ Cygni, Alpha Lacertae, 4 Lacertae, Pi² Cygni, HD 206267, Epsilon Cephei, Beta Lacertae, Sigma Ca... | 11,055 | zeroshot-train |
SGR 1900+14 [SEP] constellation | SGR 1900+14
SGR 1900+14 is a soft gamma repeater (SGR), located in the constellation of Aquila about 20,000 light-years away. It is assumed to be an example of an intensely magnetic star, known as a magnetar. It is thought to have formed after a fairly recent supernova explosion.
An intense gamma-ray burst from this st... | down its rotation. In 1998, she made careful comparisons of the periodicity of soft gamma repeater SGR 1806-20. The period had increased by 0.008 seconds since 1993, and she calculated that this would be explained by a magnetar with a magnetic-field strength of 8×10 teslas (8×10 gauss). This was enough to convince the ... | 11,056 | zeroshot-train |
Sigma Serpentis [SEP] constellation | Sigma Serpentis
Sigma Serpentis, Latinized from σ Serpentis, is a star in the equatorial constellation Serpens. It is faintly visible to the naked eye with an apparent visual magnitude of +4.82. Based upon an annual parallax shift of 36.67 mas as seen from Earth, it is located 89 light years from the Sun. The star is m... | Quzlu, Kowsar
Quzlu (, also Romanized as Qūzlū and Qowzlū; also known as Kozli and Kozly) is a village in Zarjabad Rural District, Firuz District, Kowsar County, Ardabil Province, Iran. At the 2006 census, its population was 458, in 111 families.
References.
- Tageo | 11,057 | zeroshot-train |
Tau Ceti [SEP] constellation | Tau Ceti
Tau Ceti, Latinized from τ Ceti, is a single star in the constellation Cetus that is spectrally similar to the Sun, although it has only about 78% of the Sun's mass. At a distance of just under from the Solar System, it is a relatively nearby star and the closest solitary G-class star. The star appears stable,... | -Terrestrial Intelligence (SETI) and appears in some science fiction literature.
It can be seen with the unaided eye as a third-magnitude star. As seen from Tau Ceti, the Sun would be a third-magnitude star in the northern hemisphere constellation Boötes.
Name.
The name "Tau Ceti" is the Bayer designation for this star... | 11,058 | zeroshot-train |
V4641 Sagittarii [SEP] constellation | V4641 Sagittarii
V4641 Sagittarii (V4641 Sgr) is a variable X-ray binary star system in the constellation Sagittarius. It is the source of one of the fastest superluminal jets in the Milky Way galaxy.
In 1999 a violent X-ray outburst revealed it to contain a black hole. At the time, it was considered to be the closest ... | Press, 1940.
- O’Byrne, William R. (1849) "A naval biographical dictionary: comprising the life and services of every living officer in Her Majesty's navy, from the rank of admiral of the fleet to that of lieutenant, inclusive". (London: J. Murray), vol. 1.
- Powell, John Williams Damer (1930) "Bristol Privateers and S... | 11,059 | zeroshot-train |
WASP-13 [SEP] constellation | WASP-13
WASP-13 is a star in the Lynx constellation. The star is similar, in terms of metallicity and mass, to the Sun, although it is hotter and most likely older. The star was first observed in 1997, according to the SIMBAD database, and was targeted by SuperWASP after the star was observed by one of the SuperWASP te... | Air Transport Wing, Heavy, 18 Jan 1963
- 437th Military Airlift Wing, 8 Jan 1966-1 October 1991
History Stations.
- Accra Airfield, British Gold Coast, 17 Aug 1942-30 Sep 1943
- Wheelus Air Base, Libya, 20 Jul 1952-12 Apr 1954
- Charleston AFB, South Carolina, 13 Apr 1954-1 October 1991
History Aircraft.
- C-54 Skymast... | 11,060 | zeroshot-train |
Wolf 359 [SEP] constellation | Wolf 359
Wolf 359 is a red dwarf star located in the constellation Leo, near the ecliptic. At a distance of approximately 7.9 light years from Earth, it has an apparent magnitude of 13.54 and can only be seen with a large telescope. Wolf 359 is one of the nearest stars to the Sun; only the Alpha Centauri system (includ... | NGC 359
NGC 359 is an elliptical galaxy located approximately 238 million light-years from the Solar System in the constellation Cetus. It was discovered on September 2, 1864, by Albert Marth. It was described by Dreyer as "extremely faint, very small."
See also.
- Elliptical galaxy
- List of NGC objects (1–1000)
- Cet... | 11,061 | zeroshot-train |
Zeta Delphini [SEP] constellation | Zeta Delphini
Zeta Delphini (ζ Delphini) is a star in the constellation of Delphinus. With an apparent magnitude of about 4.6, it is faintly visible to the naked eye. Parallax measurements of the system made by the Hipparcos spacecraft put it at a distance of about 220 light-years, or 67 parsecs.
Zeta Delphini has a sp... | 11500 K: Zeta Delphini has a temperature of 8336 K. Its age is estimated to be around 500 million light years, considerably younger than the Sun.
In 2014, the discovery of a brown dwarf around Zeta Delphini was announced. Zeta Delphini B is a brown dwarf with a spectral type of L5 (but may be from L3 to L7), and has a ... | 11,062 | zeroshot-train |
Zeta Ursae Minoris [SEP] constellation | Zeta Ursae Minoris
Zeta Ursae Minoris (ζ UMi, ζ Ursae Minoris) is a star in the constellation Ursa Minor. It is a white stellar class A-type main sequence star with an apparent magnitude of +4.28. It is approximately 380 light years from Earth.
Despite its classification as a main sequence dwarf star, Zeta UMi is 3.4 t... | Ahfa al Farkadain is traditionally applied to Zeta Ursae Minoris). Gamma Ursae Minoris was mostly called "Pherkad Major" to distinguish it from "Pherkad Minor" (11 Ursae Minoris). In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for s... | 11,063 | zeroshot-train |
1 Serpentis [SEP] constellation | 1 Serpentis
1 Serpentis (1 Ser) is a star in the constellation Virgo. Its apparent magnitude is 5.52. | Gamma Serpentis
Gamma Serpentis (γ Serpentis, γ Ser) is a star in the equatorial constellation Serpens, in the part of the constellation that represents the serpent's head (Serpens Caput). It has an apparent visual magnitude +3.85, which means it is visible to the naked eye. Based upon parallax measurements by the Hipp... | 11,064 | zeroshot-train |
11 Comae Berenices b [SEP] constellation | 11 Comae Berenices b
11 Comae Berenices b, (11 Com b) is an extrasolar planet orbiting the star 11 Comae Berenices, approximately 360.79lys away in the constellation of Coma Berenices. It is a massive planet with an estimated minimum mass of 19.4 Jupiters with an orbit around its parent star of 1.29AU. It was discovere... | Comae Berenices class of variable stars and the star in which the "flip-flop phenomenon" was discovered. FS Comae Berenices is a semi-regular variable, a red giant with a period of about two months whose magnitude varies between 6.1 and 5.3. R Comae Berenices is a Mira variable with a maximum magnitude of almost 7. The... | 11,065 | zeroshot-train |
15 Arietis [SEP] constellation | 15 Arietis
15 Arietis (abbreviated 15 Ari) is a single variable star in the northern constellation of Aries. "15 Arietis" is the Flamsteed designation; it also bears the variable star designation AV Arietis. It has an apparent visual magnitude of 5.74, which is just bright enough to be visible to the naked eye from dar... | Sea Fleet, North (Bei, 北) for North Sea Fleet, and South (Nan, 南) for South Sea Fleet. However, the pennant numbers may have changed due to the change of Chinese naval ships naming convention. Specification:
- Length (m): 45.7
- Beam (m): 9.5
- Draft (m): 4.6
- Standard displacement (t): 795
- Full displacement (t): 89... | 11,066 | zeroshot-train |
15 Boötis [SEP] constellation | 15 Boötis
15 Boötis is a binary star system in the northern constellation of Boötes, located approximately 260 light years away from the Sun. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.45. The system has a relatively high proper motion, traversing the celestial sphe... | Quadrans Muralis" and shrank the constellation a little in his 1801 "Uranographia" star atlas, to avoid it clashing with neighboring constellations.
In 1922, Quadrans Muralis was omitted when the International Astronomical Union (IAU) formalised its list of officially recognized constellations.
Notable features.
- The ... | 11,067 | zeroshot-train |
25 Aquarii [SEP] constellation | 25 Aquarii
25 Aquarii (abbreviated 25 Aqr) is a single star in the equatorial constellation of Aquarius. "25 Aquarii" is the modern Flamsteed designation; in the past it held the designation 6 Pegasi. It also bears the Bayer designation of d Aquarii. It is located near the border with the modern Pegasus constellation. ... | 3, and 4 Aquarii. The 11th lunar mansion shared its name with the constellation "Xu" ("emptiness"), formed by Beta Aquarii and Alpha Equulei; it represented a bleak place associated with death and funerals. "Wei", the rooftop and 12th lunar mansion, was a V-shaped constellation formed by Alpha Aquarii, Theta Pegasi, an... | 11,068 | zeroshot-train |
44 Boötis [SEP] constellation | 44 Boötis
44 Boötis or i Boötis is a triple star system in the constellation Boötes. It is approximately 41.6 light years from Earth.
The primary component, 44 Boötis A, is a yellow-white G-type main sequence dwarf with a mean apparent magnitude of +4.83. The companion component, 44 Boötis B, is a W Ursae Majoris varia... | Quadrans Muralis" and shrank the constellation a little in his 1801 "Uranographia" star atlas, to avoid it clashing with neighboring constellations.
In 1922, Quadrans Muralis was omitted when the International Astronomical Union (IAU) formalised its list of officially recognized constellations.
Notable features.
- The ... | 11,069 | zeroshot-train |
52 Cygni [SEP] constellation | 52 Cygni
52 Cygni is a giant star in the northern constellation of Cygnus with an apparent magnitude of 4.22. Based on its Hipparcos parallax, it is about away.
52 Cygni is a probable horizontal branch (red clump) star, fusing helium in its core, although there is a 25% chance that it is still on the red giant branch (... | NGC 6940
NGC 6940 is an open cluster in the constellation Vulpecula. It was discovered by William Herschel in 1784. The cluster is nearly a billion years old and it is located 2,500 light years away. It is considered the finest open cluster in the constellation.
Observation.
It is located a bit more than two degrees so... | 11,070 | zeroshot-train |
60 Arietis [SEP] constellation | 60 Arietis
60 Arietis is a star in the northern constellation of Aries. "60 Arietis" is the Flamsteed designation. It has an apparent visual magnitude of 6.14, making it a challenge to view with the naked eye. Based upon an annual parallax shift of , this star is located away from the Sun. It is receding from the Earth... | craters have undergone topographic adjustment due to isostatic phenomena (Schaber and others, 1977). This adjustment may have been facilitated by a high-temperature mantle that was conducive to “crustal plasticity” (Malin and Dzurisin, 1977). The lesser amount of intermediate plains material indicates decreasing plains... | 11,071 | zeroshot-train |
94 Aquarii [SEP] constellation | 94 Aquarii
94 Aquarii (abbreviated 94 Aqr) is a triple star system in the equatorial constellation of Aquarius. "94 Aquarii" is the Flamsteed designation. The brightest member has an apparent visual magnitude of 5.19, making it visible to the naked eye. An annual parallax shift of 47.35 milliarcseconds yields a distanc... | 3, and 4 Aquarii. The 11th lunar mansion shared its name with the constellation "Xu" ("emptiness"), formed by Beta Aquarii and Alpha Equulei; it represented a bleak place associated with death and funerals. "Wei", the rooftop and 12th lunar mansion, was a V-shaped constellation formed by Alpha Aquarii, Theta Pegasi, an... | 11,072 | zeroshot-train |
Alpha Monocerotis [SEP] constellation | Alpha Monocerotis
Alpha Monocerotis, Latinized from α Monocerotis, is the Bayer designation for the brightest star in the equatorial constellation of Monoceros. It can be viewed with the naked eye, having an apparent visual magnitude of 3.94. Based upon an annual parallax shift of 22.07 mas as seen from Earth, it is lo... | the daughter of a scientist, under the employ of Glock (Clement von Franckenstein), who is being forced to develop a nerve gas for a Latin American despot. Before the American Ninja and Hiro can rescue Lisa and her father from "Viper", the mysterious ninja that appears and reappears with a puff of smoke, the American N... | 11,073 | zeroshot-train |
CL0024+17 [SEP] constellation | CL0024+17
The cluster CL0024+17 is a cluster of galaxies located in Pisces, and about 4 billion light years distant.
Cl 0024+17 is allowing astronomers to probe the distribution of dark matter in space. The blue streaks near the center of the image are the smeared images of very distant galaxies that are not part of t... | : Hubble pictures of CL0024+17 group
- Press release and more images and video presentations of CL0024+17 at Spacetelescope.org | 11,074 | zeroshot-train |
California Nebula [SEP] constellation | California Nebula
The California Nebula (NGC 1499) is an emission nebula located in the constellation Perseus. It is so named because it appears to resemble the outline of the US State of California on long exposure photographs. It is almost 2.5° long on the sky and, because of its very low surface brightness, it is ex... | Red Square Nebula
The Red Square Nebula is a celestial object located in the area of the sky occupied by star MWC 922 in the constellation Serpens. The first images of this bipolar nebula, taken using the Mt. Palomar Hale telescope in California, were released in April 2007. It is notable for its square shape, which ac... | 11,075 | zeroshot-train |
Furuhjelm 46 [SEP] constellation | Furuhjelm 46
Furuhjelm 46, also known as HD 155876 and Gliese 661, is a nearby binary star system, consisting of two very similar red dwarfs, located in the constellation Hercules.
Furuhjelm 46 is the nearest "true" (i. e. not brown dwarf) star system in Hercules, however, there is brown dwarf in this constellation, lo... | Karl Harald Felix Furuhjelm
Karl Harald Felix Furuhjelm, () was a Governor of the Siberian specific department, in Nakhodka.
Harald Furuhjelm was born into a Swedish-speaking noble family of Furuhjelm in Helsinki, Grand Duchy of Finland on May 13, 1830. Johan Hampus was the son of Otto Wilhelm Furuhjelm (1794–1871) and... | 11,076 | zeroshot-train |
Gamma Apodis [SEP] constellation | Gamma Apodis
Gamma Apodis (γ Aps, γ Apodis) is the Bayer designation for a star in the southern circumpolar constellation of Apus. From parallax measurements, the distance to this star can be estimated as . It is visible to the naked eye with an apparent visual magnitude of 3.86. A stellar classification of G9 III iden... | The FEC argued that the Committee violated this provision when purchasing a radio advertisement that attacked the likely candidate of the Colorado Democratic Party. The court held that since the expenditures by the Committee were made independently from a specific candidate, they did not violate the campaign contributi... | 11,077 | zeroshot-train |
Gliese 832 c [SEP] constellation | Gliese 832 c
Gliese 832 c (also known as Gl 832 c or GJ 832 c) is an extrasolar planet located approximately 16 light-years (4.93 parsecs, or about 151,400,000,000,000 km) away in the constellation of Grus, orbiting the star Gliese 832, a red dwarf. It is in its star's habitable zone and a big reason for its high ratin... | The net result would be that Gliese 832 c being a desert planet, rather than an ocean planet.
Discovery and impact.
Gliese 832 c was discovered by an international team of astronomers led by Robert A. Wittenmyer. It is the newest and closest to earth member of the top three most Earth-like worlds in the Habitable Exopl... | 11,078 | zeroshot-train |
HAT-P-4b [SEP] constellation | HAT-P-4b
HAT-P-4b is a confirmed extrasolar planet orbiting the star HAT-P-4 over 1000 light years away in Boötes constellation. It was discovered by transit on October 2, 2007, which looks for slight dimming of stars caused by planets that passed in front of them. It is the fourth planet discovered by the HATNet Proje... | HAT-P-5b
HAT-P-5b is a transiting extrasolar planet located approximately 1000 light-years away in the constellation of Lyra, orbiting the star HAT-P-5. It is a hot Jupiter with a mass 6% greater than Jupiter and a radius 26% greater than Jupiter, corresponding to a density of 0.66 g/cm, which is less than water. This ... | 11,079 | zeroshot-train |
HD 125040 [SEP] constellation | HD 125040
HD 125040 is a visual binary star in the northern constellation Boötes. The pair orbit each other with a semi-major axis of 105 astronomical units and a period of roughly 750 years.
External links.
- HR 5346
- CCDM J14165+2007
- Image HD 125040 | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,080 | zeroshot-train |
HD 125612 [SEP] constellation | HD 125612
HD 125612 is a yellow main sequence star located approximately 188 light years away in the constellation Virgo. It is rich in heavy elements and has three known planets in orbit around it. A red dwarf companion star was detected in 2009 at a projected separation of 4750 AU. The possibility of a much closer co... | HD 170469
HD 170469 is a yellow subgiant star located approximately 212 light-years away in the constellation Ophiuchus. It has apparent magnitude +8.21 and it is 211.91 ly away.
In 2007, a planet was discovered by the N2K Consortium, led by principal investigators Debra Fischer and Gregory P. Laughlin.
See also.
- HD ... | 11,081 | zeroshot-train |
HD 125628 [SEP] constellation | HD 125628
HD 125628 is a double star in the constellation Centaurus. Its apparent magnitude is 4.92. | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,082 | zeroshot-train |
HD 126614 [SEP] constellation | HD 126614
HD 126614 is a 9th magnitude trinary star located approximately 240 light years away in the constellation Virgo. HD 126614 A is a K-type star while HD 126614 B and NLTT 37349 are M-type stars. Star A is larger, cooler, brighter, and more massive than our Sun. Also its metal content is 3.6 times as much as the... | HD 24496
HD 24496 is a 7th magnitude G-type wide binary star and M-type located approximately 67 light years away in the constellation Taurus. This star is smaller, cooler, fainter, and less massive than our Sun. Also its metal content is just 2% greater than the Sun. In 2009, a gas giant planet was discovered of HD 24... | 11,083 | zeroshot-train |
HD 132563 [SEP] constellation | HD 132563
HD 132563 is a triple star system in the constellation Boötes. The two resolvable components of this system are designated HD 132563A and HD 132563B. The primary star, HD 132563A, is actually a spectroscopic binary with a period of more than 15 years and an orbital eccentricity of greater than 0.65. The small... | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,084 | zeroshot-train |
HD 136118 [SEP] constellation | HD 136118
HD 136118 is a F-type main-sequence star located approximately 171 light-years away in the constellation of Serpens Cauda. It is an F-type dwarf and has apparent magnitude +6.94.
Brown dwarf companion.
The astronomer Debra Fischer discovered a very massive planet, which was announced on February 7, 2002. On N... | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,085 | zeroshot-train |
HD 152079 [SEP] constellation | HD 152079
HD 152079 is a star in the constellation Ara and has one planet.
See also.
- HD 129445
- HD 164604
- HD 175167
- HD 86226
- List of extrasolar planets | HD 86226
HD 86226 is a G type yellowish white star found in the constellation of Hydra.
Due to the reactions it had when placed under a Doppler test, 13 Magellan Doppler Velocity observations were made of an object found near the star. The object had a Keplerian orbit, was declared an exoplanet and dubbed HD 86226 b.
S... | 11,086 | zeroshot-train |
HD 153261 [SEP] constellation | HD 153261
HD 153261 is the Henry Draper Catalogue designation for a star in the southern constellation of Ara. It has an apparent visual magnitude of 6.137, placing it near the threshold of naked eye visibility. According to the Bortle Dark-Sky Scale, it can be viewed from dark suburban or rural skies. Based upon an an... | B2 IVne, indicating that it is either a main sequence or a subgiant star. The 'n' indicates a nebulous spectrum created by the Doppler shift-broadened absorption lines from a rapid rotation, while the 'e' means this is a Be star, with the spectrum showing emission lines from hot, circumstellar gas. HD 153261 display so... | 11,087 | zeroshot-train |
HD 17156 c [SEP] constellation | HD 17156 c
HD 17156 c is a plausible extrasolar planet approximately 255 light-years away in the constellation of Cassiopeia. The planet is thought to be orbiting the yellow giant star HD 17156. This planet has a mass of 0.063 Jupiter mass (or 20 Earth masses) and takes about 111.314 days or 0.305 year to orbit the sta... | HD 170469
HD 170469 is a yellow subgiant star located approximately 212 light-years away in the constellation Ophiuchus. It has apparent magnitude +8.21 and it is 211.91 ly away.
In 2007, a planet was discovered by the N2K Consortium, led by principal investigators Debra Fischer and Gregory P. Laughlin.
See also.
- HD ... | 11,088 | zeroshot-train |
HD 171978 [SEP] constellation | HD 171978
The star HD 171978 is a spectroscopic binary in the constellation of Serpens. It consists of two A-type main sequence stars orbiting each other with a period of approximately 14.7 days. The overall apparent visual magnitude of the system varies between 5.74 and 5.86. | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,089 | zeroshot-train |
HD 176527 [SEP] constellation | HD 176527
HD 176527 is a 5th magnitude star in the constellation Lyra, approximately 350 light years away from Earth. It is an orange giant star of the spectral type K2III. It therefore has a surface temperature of 3,500 to 5,000 kelvins and is much larger and brighter, yet cooler, than our Sun. | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,090 | zeroshot-train |
HD 180450 [SEP] constellation | HD 180450
HD 180450 is a 6th magnitude star in the constellation Lyra, approximately 1,400 light years away from Earth. It is a red giant star of the spectral type M0III, meaning it has a surface temperature of about 3,500 kelvins. It is much larger and brighter, yet cooler, than our Sun. It is also a star in a star cl... | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,091 | zeroshot-train |
HD 192263 [SEP] constellation | HD 192263
HD 192263 is an 8th magnitude star about 64 light years away in the constellation of Aquila. The spectral type of the star is K2V, meaning that it is an orange dwarf, a type of star somewhat cooler and less luminous than the Sun. It is not visible to the unaided eye, but with good binoculars or small telescop... | HD 192263 b
HD 192263 b is a gas giant planet with a mass about three quarters that of Jupiter mass. It orbits the star in a circular orbit completing one revolution in 24 days or so. It was discovered in 2000 by the Geneva Extrasolar Planet Search team.
In 2002 the existence of the planet was questioned by G. Henry: T... | 11,092 | zeroshot-train |
HD 210702 [SEP] constellation | HD 210702
HD 210702 is an orange subgiant star located approximately 179 light-years away in the constellation of Pegasus. With a mass of 1.8 times that of the Sun, the star spent its main-sequence life as an A-type star. The visual luminosity is 11.38 times that of the Sun and it is 182.4 light years away. The magnitu... | HD 192699
HD 192699 is a yellow subgiant star located approximately 214 light-years away in the constellation of Aquila. It has the apparent magnitude of 6.45. Based on its mass of 1.68 solar, it was an A-type star when it was a main-sequence. In April 2007, a planet was announced orbiting the star, together with HD 17... | 11,093 | zeroshot-train |
HD 210702 b [SEP] constellation | HD 210702 b
HD 210702 b is an exoplanet located approximately 182 light-years away in the constellation of Pegasus, orbiting the star HD 210702. This planet, together with HD 175541 b and HD 192699 b, are planets around intermediate mass stars that were announced in April 2007 by Johnson et al. It has at least twice th... | HD 192699
HD 192699 is a yellow subgiant star located approximately 214 light-years away in the constellation of Aquila. It has the apparent magnitude of 6.45. Based on its mass of 1.68 solar, it was an A-type star when it was a main-sequence. In April 2007, a planet was announced orbiting the star, together with HD 17... | 11,094 | zeroshot-train |
HD 214448 [SEP] constellation | HD 214448
HD 214448 is a binary star system in the equatorial constellation of Aquarius. They orbit each other with a period of around 147 years. The combined mass of the pair is twice that of the Sun.
External links.
- Image HD 214448 | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,095 | zeroshot-train |
HD 28185 [SEP] constellation | HD 28185
HD 28185 is a yellow dwarf star similar to our Sun located about 128.6 light-years away from Earth in the constellation Eridanus. The designation HD 28185 refers to its entry in the Henry Draper catalogue. The star is known to possess one long-period extrasolar planet.
Distance and visibility.
According to mea... | and that three of them are in the habitable zone.
Description (alphabetical order) HD 28185 b.
HD 28185 b was the first exoplanet to be detected in the habitable zone. The planet has only been detected indirectly, but is believed to be a gas giant, with no solid surface. Some scientists have argued that it could have m... | 11,096 | zeroshot-train |
HD 33463 [SEP] constellation | HD 33463
HD 33463 is a suspected variable star in the northern constellation of Auriga. This is a red giant star with a stellar classification of M2III.
External links.
- HIC 24193
- Image HD 33463 | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,097 | zeroshot-train |
HD 34626 [SEP] constellation | HD 34626
HD 34626, also known as MZ Aurigae, is an unusual variable star in the northern constellation of Auriga. It varies in brightness by 0.1 magnitude over time scales of 8 to 12 hours, but these variations are not periodic. This indicates the variability is not caused by ellipsoidal effects, and the nature of the ... | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,098 | zeroshot-train |
HD 43691 b [SEP] constellation | HD 43691 b
HD 43691 b is a massive jovian planet located approximately 280 light-years away in the constellation of Auriga. Because the inclination is unknown, only the minimum mass is known. The planet orbits close to the star, closer than Mercury to the Sun. | , a G5IV type star 49 parsecs away. It has a mass of 1.02 solar masses and a radius of 1.27 solar radii. HD 43691 b is a significantly larger planet, with a mass of 2.49 Jupiter masses; it is also far closer to its parent star, HD 43691. Discovered in 2007 from radial velocity measurements, it orbits at a distance of 0... | 11,099 | zeroshot-train |
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