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HD 147018 b [SEP] constellation | HD 147018 b
HD 147018 b is a gas giant extrasolar planet which orbits the G-type main sequence star HD 147018, located approximately 140 light years away in the constellation Triangulum Australe. This planet has minimum mass more than twice that of Jupiter but this planet orbits a lot closer to the star than Jupiter to... | HD 171238
HD 171238 is a 9th magnitude G-type main sequence star located approximately 146 light years away in the constellation Sagittarius. This star is a little bit cooler, less massive, older, and more metallic than the Sun. In August 2009, it was announced that this star has a planet.
See also.
- HD 147018
- HD 20... | 11,700 | zeroshot-train |
HD 147513 [SEP] constellation | HD 147513
HD 147513 (62 G. Scorpii) is a star in the southern constellation of Scorpius. It was first catalogued by Italian astronomer Piazzi in his star catalogue as "XVI 55". With an apparent magnitude of 5.38, according to the Bortle scale it is visible to the naked eye from suburban skies. Based upon stellar parall... | of G1VH-04. It has about 11% greater mass than the Sun, and is considered young with an estimated age of 400 million years. As such, it has a similar luminosity to the Sun despite being more massive. Although the abundance of elements is similar to the Sun, it is a Barium star that is overabundant in elements produced ... | 11,701 | zeroshot-train |
HD 151566 [SEP] constellation | HD 151566
HD 151566 is double star in the southern constellation of Ara. As of 1991, the pair had an angular separation of 3.10″ along a position angle of 42°.
External links.
- HR 6236
- CCDM J16506-5003
- Image HD 151566 | 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-... | 11,702 | zeroshot-train |
HD 152010 [SEP] constellation | HD 152010
HD 152010 is a star in the southern constellation of Apus.
External links.
- Image HD 152010 | 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-... | 11,703 | zeroshot-train |
HD 153791 [SEP] constellation | HD 153791
HD 153791 is a double star in the southern constellation of Ara. The primary is a sixth magnitude A-type main sequence star. It has a magnitude 12.3 companion at an angular separation of 6.0″ along a position angle of 249°, as of 1999.
External links.
- HR 6323
- CCDM J17037-4710
- Image HD 153791 | 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-... | 11,704 | zeroshot-train |
HD 168625 [SEP] constellation | HD 168625
HD 168625 (V4030 Sagittarii) is a blue hypergiant and candidate luminous blue variable located in the constellation of Sagittarius easy to see with amateur telescopes. It forms a visual pair with the also blue hypergiant (and luminous blue variable) HD 168607 and is located to the south-east of M17, the Omega... | association Serpens OB1, at a distance to the Sun of 2.2 kiloparsecs (7.200 light years), others think HD 168625 is farther, at a distance estimated to be 2.8 kiloparsecs (kpc) (9,100 light years) and unrelated to the former objects. The parallax published in Gaia Data Release 2 indicates a distance close to 1,600 pc, ... | 11,705 | zeroshot-train |
HD 174179 [SEP] constellation | HD 174179
HD 174179 is a 6th magnitude star in the constellation Lyra, approximately 1,100 light years from Earth. It is a bluish white subgiant star of the spectral type B3IVp, meaning it possesses a surface temperature of 11,000 to 25,000 kelvins. Its surface is at least twice as hot as the Sun, and it is larger and ... | 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-... | 11,706 | zeroshot-train |
HD 23079 b [SEP] constellation | 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... | 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... | 11,707 | zeroshot-train |
HD 35984 [SEP] constellation | HD 35984
HD 35984 is star in the northern constellation Auriga. It has an apparent magnitude of 6.20, which, according to the Bortle scale, indicates it is faintly visible to the naked eye from dark rural skies. Parallax measurements by the Hipparcos satellite indicates it lies at a distance of roughly 290 light years ... | levels of lithium may indicate that this is instead a weak-lined T Tauri star. That is, a low mass pre-main sequence star that is relatively poor in circumstellar matter.
External links.
- HR 1822
- Image HD 35984 | 11,708 | zeroshot-train |
HD 45184 [SEP] constellation | HD 45184
HD 45184 is a 6th magnitude G-type main sequence star located approximately 71 light years away in the constellation Canis Major. It has a planet around 12 times as massive as Earth that takes 5.88 days to complete an orbit around its host star. The planet was detected by radial velocity.
See also.
- List of e... | 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-... | 11,709 | zeroshot-train |
HD 57821 [SEP] constellation | HD 57821
HD 57821 is a star in the constellation Canis Major. Its apparent magnitude is 4.96. | 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-... | 11,710 | zeroshot-train |
HD 70642 [SEP] constellation | HD 70642
HD 70642 is a yellow dwarf star in the constellation of Puppis located 92 light years away. This star has about the same mass and radius as the Sun, is slightly cooler and less luminous, and is richer in abundance of iron relative to hydrogen.
Planetary system.
A long period planet companion to HD 70642 was an... | HD 47186 b
HD 47186 b is a “hot Neptune” extrasolar planet located approximately 123 light years away in the constellation of Canis Major, orbiting the star HD 47186. This planet has a minimum mass of 22.78 times that of Earth and orbits very close to the star at a similar distance from the star as 51 Pegasi b is from ... | 11,711 | zeroshot-train |
HD 86081 [SEP] constellation | HD 86081
HD 86081 is a yellow-white dwarf star in the constellation Sextans south of the celestial equator. It is bigger and more massive than our Sun at 1.22 and 1.21 solar units respectively. It has temperature of 6028 K and luminosity of 1.75 solar.
HD 86081 shows no evidence of planetary transits in spite of a 17.6... | HD 86081 b
HD 86081 b is a gas giant exoplanet that orbits close to its host star, completing its orbit for only 2.1375 days. With such a short orbit, it belongs to the class of exoplanets known as hot Jupiters. Like most hot Jupiters, the orbit is nearly circular, with an eccentricity of 0.008. | 11,712 | zeroshot-train |
HD 90089 [SEP] constellation | HD 90089
HD 90089 is a suspected variable star in the constellation Camelopardalis.
An infrared excess has been detected around this star, most likely indicating the presence of a circumstellar disk at a radius of 145 AU. The temperature of this dust is 30 K.
References.
- HR 4084
- Image HD 90089 | 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-... | 11,713 | zeroshot-train |
HD 91942 [SEP] constellation | HD 91942
HD 91942, also known as r Carinae (r Car), is a star in the constellation Carina. r Carinae is an orange K-type bright giant with an apparent magnitude of +4.45. It is approximately 1380 light years from Earth. | 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-... | 11,714 | zeroshot-train |
HD 92063 [SEP] constellation | HD 92063
HD 92063, also known as t¹ Carinae (t¹ Car), is a star in the constellation Carina. t¹ Carinae is an orange K-type giant with an apparent magnitude of +5.08. It is approximately 269 light years from Earth. | 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-... | 11,715 | zeroshot-train |
HIP 14810 b [SEP] constellation | HIP 14810 b
HIP 14810 b is a massive hot Jupiter approximately 165 light-years away in the constellation of Aries. It has mass 3.88 times that of Jupiter and orbits at 0.0692 AU. It was discovered by the N2K Consortium in 2006 and the discovery paper was published in 2007. Prior to this a preliminary orbit had been pub... | & Richard Greenberg, Lunar and Planetary Lab, University of Arizona
- Image HIP 14810 | 11,716 | zeroshot-train |
HIP 57274 [SEP] constellation | HIP 57274
HIP 57274 is a star in the constellation Ursa Major. Its apparent magnitude is 8.96. Three planets orbit it. | HIP 57274 d
HIP 57274 d is an exoplanet orbiting the K-type main sequence star HIP 57274 about 84.5 light-years (26 parsecs, or nearly km) from Earth in the constellation Cetus. It orbits within the outer part of its star's habitable zone, at a distance of 1.01 AU. The exoplanet was found by using the radial velocity m... | 11,717 | zeroshot-train |
HIP 79431 [SEP] constellation | HIP 79431
HIP 79431 is an 11th magnitude M-type main sequence star located approximately 47 light years away in the constellation Scorpius. This star is smaller, cooler, dimmer, and less massive than our Sun. Also its metal content is 2.5 times as much as the Sun. In 2010, a superjovian planet was found in orbit around... | Gliese 179
Gliese 179 is a 12th magnitude M-type main sequence star located approximately 40 light years away in the constellation Orion. This star is smaller, cooler, fainter, and less massive than our Sun. Also its metal content is twice as much as the Sun. In 2009, a gas giant planet was found in orbit around the st... | 11,718 | zeroshot-train |
HR 6806 [SEP] constellation | HR 6806
HR 6806 is a solitary, orange, main sequence (K2 V) star located thirty-six light-years away, in the constellation Hercules. The star is smaller than the Sun, with around 79% of the solar mass and radius, and 35% of the solar luminosity. It appears to be rotating slowly with an estimated period of 42 days. The ... | J180901.07+383805.4, at an angular separation of 769″, which would correspond to a projected separation of 8460 AU at the distance of HR 6806. However, this is most likely a typical T7 dwarf, which would place it at a distance of —ruling out a physical association. This is confirmed by the differing proper motion of th... | 11,719 | zeroshot-train |
IOK-1 [SEP] constellation | IOK-1
IOK-1 is a distant galaxy in the constellation Coma Berenices. When discovered in 2006, it was the oldest and most distant galaxy ever found, at redshift 6.96.
It was discovered in April 2006 by Masanori Iye at National Astronomical Observatory of Japan using the Subaru Telescope in Hawaii and seen as it was 12.8... | 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... | 11,720 | zeroshot-train |
IRAS 17163-3907 [SEP] constellation | IRAS 17163−3907
IRAS 17163−3907, also known as Hen 3-1379, is a possible yellow hypergiant star located 13,000 light years from Earth in the constellation of Scorpius. The star is embedded in thick shells of expelled gases and dust, and owing to its appearance has been nicknamed by astronomers the "Fried Egg Nebula". Y... | - V509 Cassiopeiae
- IRC+10420 (V1302 Aql)
- IRAS 18357-0604
- V766 Centauri (= HR 5171A) (possibly a red supergiant)
- HD 179821
- IRAS 17163-3907
- V382 Carinae
- RSGC1-F15
In Westerlund 1:
- W4
- W8a
- W12a
- W16a
- W32
- W265
In other galaxies:
- HD 7583 (R45 in SMC)
- HD 33579 (in LMC)
- HD 269723 (R117 in | 11,721 | zeroshot-train |
Iota Ceti [SEP] constellation | Iota Ceti
Iota Ceti (ι Cet, ι Ceti) is the Bayer designation for a star system in the equatorial constellation of Cetus. It has the traditional name Deneb Kaitos Shemali. The name was from the Arabic word ذنب قيطس الشمالي - "dhanab qayṭas al-shamālī", meaning "the northern tail of the sea monster". it is visible to the... | Thalath Al Naamat), and Upsilon Ceti, formed "Al Naʽāmāt" ('ألنعامة), "the Hen Ostriches".
In Chinese, (), meaning "Square Celestial Granary", refers to an asterism consisting of Zeta Ceti, Iota Ceti, Theta Ceti, Eta Ceti, Tau Ceti and 57 Ceti. Consequently, the Chinese name for Zeta Ceti itself is (, ).
Properties.
Ze... | 11,722 | zeroshot-train |
Kappa1 Coronae Australis [SEP] constellation | Kappa1 Coronae Australis
Kappa Coronae Australis (κ CrA), is a star located in the constellation Corona Australis. It forms a line-of-sight double star along with κ Coronae Australis. κ Coronae Australis is also known as HR 6952 and HD 170868. κ Coronae Australis is also known as HR 6953, and is located 21.4 arcminutes... | as Kappa1 is much more distant than the dimmer and closer Kappa2. Kappa2 Coronae Australis is a B9V star with apparent a visual magnitude of +5.65 and an absolute magnitude of +0.421.
Kappa2 Coronae Australis is located at a distance of 150 pc or 488.4 light years.
External links.
- Alcyone.de
- Alcyone.de
- Simbad.u-s... | 11,723 | zeroshot-train |
Kepler-8b [SEP] constellation | Kepler-8b
Kepler-8b is the fifth of the first five exoplanets discovered by NASA's Kepler spacecraft, which aims to discover planets in a region of the sky between the constellations Lyra and Cygnus that transit (cross in front of) their host stars. The planet is the hottest of the five. Kepler-8b was the only planet d... | of Kepler-6b behind its star.
The confirmation of Kepler-6b was announced at the 215th meeting of the American Astronomical Society with the discoveries of planets Kepler-4b, Kepler-5b, Kepler-7b, and Kepler-8b on January 4, 2010.
Host star.
Kepler-6 is a sunlike star in the Cygnus constellation. It is approximately 20... | 11,724 | zeroshot-train |
Kepler-9 [SEP] constellation | Kepler-9
Kepler-9 is a sunlike star in the constellation Lyra. Its planetary system, discovered by the Kepler Mission in 2010 was the first detected with the transit method found to contain multiple planets.
Nomenclature and history.
Kepler-9 was named for the Kepler Mission, a project headed by NASA that was designed ... | discovered with more than three transiting planets, and is also part of the most compact and flat system yet discovered. Kepler-11's planetary system is the second known system to have multiple transiting planets, surpassing the three confirmed planets (two transiting) orbiting the star Kepler-9.
Host star.
Kepler-11 i... | 11,725 | zeroshot-train |
Messier 19 [SEP] constellation | Messier 19
Messier 19 or M19 (also designated NGC 6273) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier on June 5, 1764 and added to his catalogue of comet-like objects that same year. It was resolved into individual stars by William Herschel in 1784. His son, John Herschel, d... | Messier 47
Messier 47 (M47 or NGC 2422) is an open cluster in the constellation Puppis. It was discovered by Giovanni Batista Hodierna before 1654 and independently discovered by Charles Messier on February 19, 1771. It was later independently discovered again, under the current name NGC 2422.
There is actually no clus... | 11,726 | zeroshot-train |
Messier 80 [SEP] constellation | Messier 80
Messier 80 (also known as M80 or NGC 6093) is a globular cluster in the constellation Scorpius. It was discovered by Charles Messier in 1781.
The star cluster is located midway between α Scorpii (Antares) and β Scorpii in a field in the Milky Way that is rich in nebulae. It can be viewed with modest amateur ... | Messier 56
Messier 56 (also known as M56 or NGC 6779) is a globular cluster in the constellation Lyra. It was discovered by Charles Messier on January 19, 1779. The cluster is located almost midway along an imaginary line between Albireo (β Cygni) and Sulafat (γ Lyrae). It is a challenge to find with large (50–80 mm) b... | 11,727 | zeroshot-train |
Messier 88 [SEP] constellation | Messier 88
Messier 88 (also known as M88 or NGC 4501) is a spiral galaxy about 50 to 60 million light-years away in the constellation Coma Berenices. It was discovered by Charles Messier in 1781.
Properties.
M88 is one of the fifteen Messier objects that belong to the nearby Virgo Cluster of galaxies. It is galaxy numb... | 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... | 11,728 | zeroshot-train |
NGC 1073 [SEP] constellation | 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... | galaxies of a small galaxy group that also includes NGC 1073, and five other small irregular galaxies.
NGC 1087, NGC 1090, and NGC 1094 appear close, but they simply appear in the field of view and are background galaxies.
Based on the published red shift, (Hubble Constant of 62 km/s per Mpc) a rough distance estimate ... | 11,729 | zeroshot-train |
NGC 1261 [SEP] constellation | NGC 1261
NGC 1261, also known as Caldwell 87, is a globular cluster in the constellation Horologium, first discovered by James Dunlop in 1826.
External links.
- SEDS
- NASA data
- Photometry paper
- Globular Clusters Database | 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... | 11,730 | zeroshot-train |
NGC 2022 [SEP] constellation | NGC 2022
NGC 2022 is a planetary nebula in the constellation Orion. In medium-sized amateur telescopes it looks like small grayish patch of light. It is not very bright but it is still easy to spot it in the eyepiece. It has an apparent size of 0.65 arcminutes. | characters, which form a contiguous range of code points. These codes (0x21–0x7E, as corresponding high bit set bytes 0xA1–0xFE) also used in various multi-byte encoding schemes for languages of East Asia, such as ISO 2022, EUC and GB 2312. For this reason, code pages of 94 and even 94 code points were common in East A... | 11,731 | zeroshot-train |
NGC 2291 [SEP] constellation | NGC 2291
NGC 2291 is a lenticular galaxy in the constellation Gemini. It was discovered by John Herschel on January 22, 1827. The visual magnitude is 13, and the apparent size is 1.0 by 0.8 arc minutes. | 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... | 11,732 | zeroshot-train |
NGC 2438 [SEP] constellation | NGC 2438
NGC 2438 is a planetary nebula about 3,000 light years away in the constellation Puppis. It was discovered by William Herschel on March 19, 1786.
NGC 2438 appears to lie within the cluster M46, but it is most likely unrelated since it does not share the cluster's radial velocity. The case is yet another exampl... | , NGC 2438 is a larger object in the background.
External links.
- PIA04228: Rotten Egg Nebula, NASA Planetary Photojournal
- The Rotten Egg Planetary Nebula, APOD 1999 November 1
- The Making of the Rotten Egg Nebula, APOD 2001 September 3
- Calabash Nebula at Constellation Guide
- Calabash Nebula imaged and interpre... | 11,733 | zeroshot-train |
NGC 2467 [SEP] constellation | NGC 2467
NGC 2467 is a star-forming region, popularly known as the "Skull and Crossbones nebula," whose appearance has occasionally also been likened to that of a colorful mandrill. It includes areas where large clouds of hydrogen gas incubate new stars. This region was one of the areas featured in the book "" by Teren... | .
- NGC 2467
- Star Birth NGC 2467 (Gemini Observatory) | 11,734 | zeroshot-train |
NGC 2768 [SEP] constellation | NGC 2768
NGC 2768 is a lenticular galaxy located in the constellation of Ursa Major. It is at a distance of 65 million light years from Earth. NGC 2768 is an example of a Seyfert galaxy, an object with a supermassive black hole at its centre. A dusty structure is encircling the centre of the galaxy, forming a knotted r... | the basic, global chemo-dynamical properties of early type galaxies?
2. What is the distribution of dark matter in early-type galaxies?
3. How are the outer regions of early-type galaxies assembled?
4. How does assembly depend on mass, environment, and other variables?
5. Do the observations agree with theoretical mode... | 11,735 | zeroshot-train |
NGC 3384 [SEP] constellation | NGC 3384
NGC 3384 is an elliptical galaxy in the constellation Leo. The galaxy was discovered by William Herschel in 1784 as part of the Herschel 400 Catalogue. The high age of the stars in the central region of NGC 3384 was confirmed after analysis of their color. More than 80% were found to be Population II stars whi... | black hole is listed as fourth largest, and it is unusually large in proportion to the host galaxy, being 14% of the mass, instead of the usual 0.1%
- NGC 1566
- NGC 2778
- NGC 2787
- NGC 3079
- NGC 3115
- NGC 3245
- NGC 3377
- NGC 3384
- NGC 3608
- NGC 3894
- NGC 3998
- NGC 4151
- NGC 4261
- NGC 4291
- NGC 4342
- NGC ... | 11,736 | zeroshot-train |
NGC 35 [SEP] constellation | NGC 35
NGC 35 is a spiral galaxy in the Cetus constellation. | NGC 7064
NGC 7064 is a nearby edge-on barred spiral galaxy located about 35 million light-years away in the constellation of Indus. NGC 7064 has an estimated diameter of 51,000 light-years. NGC 7064 was discovered by astronomer John Herschel on July 8, 1834.
See also.
- NGC 4013
- List of NGC objects (7001–7840) | 11,737 | zeroshot-train |
NGC 36 [SEP] constellation | NGC 36
NGC 36 is a spiral galaxy in the constellation Pisces. | NGC 4689
NGC 4689 is a spiral galaxy located about 54 million light-years away in the constellation of Coma Berenices. NGC 4689 is also classified as a LINER galaxy. NGC 4689 is inclined at an angle of about 36° which means that the galaxy is seen almost face-on to the Earth's line of sight. NGC 4689 was discovered by ... | 11,738 | zeroshot-train |
NGC 4038 Group [SEP] constellation | NGC 4038 Group
The NGC 4038 Group is a group of galaxies in the constellations Corvus and Crater. The group may contain between 13 and 27 galaxies. The group's best known galaxies are the Antennae Galaxies (NGC 4038/NGC4039), a well-known interacting pair of galaxies.
Members.
The table below lists galaxies that have b... | old, with the formation of the globulars likely originating from shockwaves, generated by the collision of the galaxies, compressing large, massive molecular clouds. The densest regions of the collapsing and compressing clouds are believed to be the birthplace of the clusters.
Timeline.
About 1.2 billion years ago, the... | 11,739 | zeroshot-train |
NGC 4700 [SEP] constellation | NGC 4700
NGC 4700 is a spiral galaxy located about 50 million light years away in the constellation of Virgo. NGC 4700 was discovered in March 1786 by the British astronomer William Herschel who noted it as a "very faint nebula".
NGC 4700 was imaged by Hubble in 2012, showing an abundance of star-forming regions simila... | NGC 708
NGC 708 is an elliptical galaxy located 240 million light-years away in the constellation Andromeda and was discovered by astronomer William Herschel on September 21, 1786. It is classified as a cD galaxy and is the brightest member of Abell 262. NGC 708 is a weak FR I radio galaxy and is also classified as a t... | 11,740 | zeroshot-train |
NGC 6366 [SEP] constellation | NGC 6366
NGC 6366 is a globular cluster located in the constellation Ophiuchus. It is designated as XI in the galaxy morphological classification scheme and was discovered by the German astronomer Friedrich August Theodor Winnecke on 12 April 1860. It is at a distance of 11,700 light years away from earth.
See also.
- ... | star in the cluster.
Slightly over 3° southwest of M14 lies the faint globular cluster NGC 6366.
External links.
- SEDS Messier pages on M14
- M14, Galactic Globular Clusters Database page
- - one of the two being M14 | 11,741 | zeroshot-train |
NGC 6818 [SEP] constellation | NGC 6818
The Little Gem Nebula or NGC 6818 is a planetary nebula located in the constellation of Sagittarius. It has magnitude 10 and oval diameter of 15 to 22 arcseconds with a 15th magnitude central star.
It was discovered by William Herschel in 1787.
NGC 6818 is located in the constellation of Sagittarius (The Arche... | , they send their outer layers into space to create glowing clouds of gas, a planetary nebulae. This ejection of mass is uneven, and planetary nebulae can have complex shapes. NGC 6818 shows knotty filament-like structures and distinct layers of material, with a bright and enclosed central bubble surrounded by a larger... | 11,742 | zeroshot-train |
NGC 7027 [SEP] constellation | NGC 7027
NGC 7027 is a very young and dense planetary nebula located around from Earth in the constellation Cygnus. Discovered in 1878 by Édouard Stephan using the reflector at Marseille Observatory, it is one of the smallest planetary nebulae and by far the most extensively studied. Helium hydride was detected in the ... | atoms are being ionized.
The expanding halo of NGC 7027 has a mass of about three times the mass of the Sun, and is about 100 times more massive than the ionized central region. This mass loss in NGC 7027 provided important evidence that stars a few times more massive than the Sun can avoid being destroyed in supernova... | 11,743 | zeroshot-train |
NGC 7537 [SEP] constellation | NGC 7537
NGC 7537 is a spiral galaxy located in the constellation Pisces. | 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... | 11,744 | zeroshot-train |
NGC 81 [SEP] constellation | NGC 81
NGC 81 is a lenticular galaxy estimated to be about 270 million light-years away in the constellation of Andromeda. | NGC 3370
NGC 3370 (also known as UGC 5887 or Silverado Galaxy) is a spiral galaxy about 98 million light-years away in the constellation Leo. It is comparable to our own Milky Way both in diameter (100,000 light years) and mass (10 solar masses). NGC 3370 exhibits an intricate spiral arm structure surrounding a poorly ... | 11,745 | zeroshot-train |
Nu Sagittarii [SEP] constellation | Nu Sagittarii
The Bayer designation Nu Sagittarii (Nu Sgr, ν Sagittarii, ν Sgr) is shared by two star systems, ν Sagittarii and ν Sagittarii, in the zodiac constellation Sagittarius. The two stars are separated by 0.23° in the sky.
- ν Sagittarii
- ν Sagittarii
Nu Sagittarii has the traditional name Ain al Rami, which ... | Nu1 Sagittarii
Nu¹ Sagittarii (ν¹ Sagittarii, abbreviated Nu¹ Sgr, ν¹ Sgr) is a triple star system lying approximately 1,100 light-years from Earth. Its three components are designated Nu¹ Sagittarii A (officially named Ainalrami , the traditional name for the system), B and C. A and B themselves form a spectroscopic b... | 11,746 | zeroshot-train |
PSR B0950+08 [SEP] constellation | PSR B0950+08
The pulsar PSR B0950+08 seems to have come from a supernova that occurred in Leo 1.8 million years ago. The remnant of this supernova may be the nearest besides the Local Bubble, and the supernova would have been as bright as the moon.
External links.
- "The Astrophysical Journal Letters", vol. 576, p. L41... | PSR B1257+12
PSR B1257+12, previously designated PSR 1257+12, alternatively designated PSR J1300+1240, also named Lich (pronounced "litch"), is a pulsar located 2,300 light-years from the Sun in the constellation of Virgo.
The pulsar has a planetary system with three known planets, named "Draugr" (PSR B1257+12 b or PSR... | 11,747 | zeroshot-train |
Palomar 6 [SEP] constellation | Palomar 6
Palomar 6 is a loose globular cluster in the constellation Ophiuchus that belongs to the halo of the Milky Way galaxy.
First discovered on the National Geographic Society – Palomar Observatory Sky Survey plates by Robert G. Harrington and Fritz Zwicky,
It was catalogued as a globular cluster. One of four glo... | have been obtained (beginning at 6 hours after the actual explosion), is the Type II SN 2013fs (iPTF13dqy) which was recorded 3 hours after the supernova event on 6 October 2013 by the Intermediate Palomar Transient Factory (iPTF). The star is located in a spiral galaxy named NGC 7610, 160 million light years away in t... | 11,748 | zeroshot-train |
Pi Ursae Minoris [SEP] constellation | Pi Ursae Minoris
The Bayer designation Pi Ursae Minoris (π UMi, π Ursae Minoris) is shared by two star systems, π Ursae Minoris and π Ursae Minoris, in the constellation Ursa Minor. They are separated by 0.64° on the sky.
- π Ursae Minoris
- π Ursae Minoris | , while his countryman Johann Elert Bode subsequently added iota to phi. Only lambda and pi remain in use, likely because of their proximity to the north celestial pole. Within the constellation's borders, there are 39 stars brighter than or equal to apparent magnitude 6.5.
Marking the Little Bear's tail, Polaris, or A... | 11,749 | zeroshot-train |
RX J0822-4300 [SEP] constellation | RX J0822−4300
RX J0822−4300, often referred to as a "Cosmic Cannonball", is a radio-quiet neutron star currently moving away from the center of the Puppis A supernova remnant at over 3 million miles per hour (5 400 000 km/h; 1500 km/s; ~0.5% the speed of light), making it one of the fastest moving stars ever found. Ast... | of the boost.
Some neutron stars are inferred to be traveling with similar speeds. This could be related to HVSs and the HVS ejection mechanism. Neutron stars are the remnants of supernova explosions, and their extreme speeds are very likely the result of an asymmetric supernova explosion or the loss of their near part... | 11,750 | zeroshot-train |
RY Sagittarii [SEP] constellation | RY Sagittarii
RY Sagittarii is a yellow supergiant and an R Coronae Borealis type variable star in the constellation Sagittarius. Although it ostensibly has the spectrum of a G-type star, it differs markedly from most in that it has almost no hydrogen and a lot of carbon.
Discovery.
Colonel Ernest Elliott Markwick firs... | of Congress in 1990. Sagir Ahmad of Congress defeated Rajnandan Rai of LD in 1985, Radha Pandey of Janata Party (JP) in 1980 and Shankar Prasad Yadav of Janata Party in 1977. | 11,751 | zeroshot-train |
Rho Aquilae [SEP] constellation | Rho Aquilae
Rho Aquilae, ρ Aquilae, is the Bayer designation for a star in the northern constellation of Delphinus. It has an apparent visual magnitude of 4.94 and is bright enough to be seen with the naked eye in good conditions.
Distance, proper motion and constellation.
Parallax shift (measured at any interval of ha... | Scorpius to Libra and given the new names Sigma and Upsilon Librae. (To add to the confusion, the star now known as Omicron Scorpii was not named by Bayer but was assigned the designation o Scorpii (Latin lower case 'o') by Lacaille – which later astronomers misinterpreted as omicron once Bayer's omicron had been reass... | 11,752 | zeroshot-train |
Rho Geminorum [SEP] constellation | Rho Geminorum
Rho Geminorum (ρ Gem) is a star system that lies approximately 59 light-years away in the constellation of Gemini, about 5 arcminutes east of Castor. The system consists of a primary bright enough to be seen with the naked eye, a faint secondary which has rarely been observed even professionally, and a di... | +3147 E (Rho Geminorum C), has a larger still separation of 756 arcseconds, translating to a separation perpendicular to the line of sight of about 18600 AU. The position of this star relative to the primary has remained consistent over decades, indicating that it has a common proper motion and is therefore a wide tert... | 11,753 | zeroshot-train |
Rho Telescopii [SEP] constellation | Rho Telescopii
Rho Telescopii (ρ Tel, ρ Telescopii) is the Bayer designation for an astrometric binary star system in the southern constellation of Telescopium. It is visible to the naked eye, with an apparent visual magnitude of +5.17. Based upon an annual parallax shift of 17.63 mas as measured from Earth, it is loca... | "Super Robot Wars" series of video games, beginning with "Super Robot Wars NEO" for the Wii along with the other 3 Eldran robots.
It also appeared in New Century Brave Wars on the PlayStation 2 in Japan to establish the first official connection between the Eldran and Yuusha series, following the merger of Takara and T... | 11,754 | zeroshot-train |
Rosette Nebula [SEP] constellation | Rosette Nebula
The Rosette Nebula (also known as Caldwell 49) is a large spherical H II region (circular in appearance) located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the stars of the clu... | Videocast on Rosette Nebula
- Rosette Nebula from the Netherlands
- Deep image of the Rosette Nebula
- The Scale of the Universe (Astronomy Picture of the Day 2012 March 12)
- Rosette Nebula at Constellation Guide | 11,755 | zeroshot-train |
SDSS J1416+1348 [SEP] constellation | SDSS J1416+1348
SDSS J1416+1348 (full designation is SDSS J141624.08+134826.7) is a nearby wide binary system of two brown dwarfs, located in constellation Boötes. The system consists of L-type component A and T-type component B.
Discovery.
Component A was discovered in late 2009 from a search of Sloan Digital Sky Surv... | indicates that SDSS J1416+1348 is now approaching to us). Total velocity of SDSS J1416+1348 relatively to Solar system is 42.8 km/s.
SDSS J1416+1348 space motions estimates
Space motion of SDSS J1416+1348 indicates that it is member of Galactic thin disk population.
Space motion Solar encounter.
Since SDSS J1416+1348 m... | 11,756 | zeroshot-train |
SGR 1627-41 [SEP] constellation | SGR 1627-41
SGR 1627-41, is a soft gamma repeater (SGR), located in the constellation of Ara. It was discovered June 15, 1998 using the Burst and transient Source Experiment (BATSE) and was the first soft gamma repeater to be discovered since 1979. During a period of 6 weeks, the star bursted approximately 100 times, a... | the 40-day afterglow, SGR 1627-41 has remained dormant and is steadily cooling down from the peak during the event.
References.
- XMM-Newton observation of the Soft Gamma Ray Repeater SGR 1627-41 in a low luminosity state | 11,757 | zeroshot-train |
SGR 1806-20 [SEP] constellation | SGR 1806−20
SGR 1806−20 is a magnetar, a type of neutron star with a very powerful magnetic field, that was discovered in 1979 and identified as a soft gamma repeater. SGR 1806−20 is located about 14.5 kiloparsecs (50,000 light-years) from Earth on the far side of the Milky Way in the constellation of Sagittarius. It h... | 10 light years) of Earth would destroy the ozone layer and be similar in effect to a 12-kiloton nuclear blast at 7.5 kilometers. The nearest known magnetar to Earth is 1E 1048.1-5937, located 9,000 light-years away in the constellation Carina.
Location.
SGR 1806−20 lies at the core of radio nebula G10.0-0.3 and is a me... | 11,758 | zeroshot-train |
SN 2008ha [SEP] constellation | SN 2008ha
SN 2008ha was a type Ia supernova which was first observed around November 7, 2008 in the galaxy UGC 12682, which lies in the constellation Pegasus at a distance of about from Earth.
SN 2008ha was unusual in several ways: with an absolute V band magnitude of −14.2 it is one of the faintest supernovae ever obs... | found supernova SN 2008ha late November 2008. At the age of 14 she had been declared the youngest person ever to find a supernova. However, in January 2011, 10-year-old Kathryn Aurora Gray from Canada was reported to have discovered a supernova, making her the youngest ever to find a supernova. Mr. Gray, her father, an... | 11,759 | zeroshot-train |
Sigma Aquarii [SEP] constellation | Sigma Aquarii
Sigma Aquarii (σ Aqr, σ Aquarii) is the Bayer designation for a double star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of 4.81. Based upon parallax measurements, the distance to this star is roughly .
Sigma Aquarii has a stellar classifica... | 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... | 11,760 | zeroshot-train |
V391 Pegasi b [SEP] constellation | V391 Pegasi b
V391 Pegasi b, also known as HS 2201+2610 b, is an extrasolar planet candidate orbiting the star V391 Pegasi approximately 4570 light-years away in the constellation of Pegasus. The candidate planet was discovered by means of variable star timing, which measured anomalies in variability of the star caused... | phase, and eventually become asymptotic giant branch stars. The reason that some stars, like V391 Pegasi, lose so much mass is not well known.
Planetary system.
In 2007, a gas giant planet designated V391 Pegasi b was found in orbit by variable star timing method. This planet around an "extreme horizontal branch" star ... | 11,761 | zeroshot-train |
WASP-18 [SEP] constellation | WASP-18
WASP-18 is a magnitude 9 star located in the Phoenix constellation of the southern hemisphere. It has a mass of 1.25 solar masses.
In 2009, the SuperWASP project announced that a large, hot Jupiter type extrasolar planet, "WASP-18b", was orbiting very close to this star.
Observations from the Chandra X-ray Obse... | Francisco Naval Shipyard (1955–58), he was responsible for the modernization (SCB-125) of World War II carriers USS "Wasp" (CV-18), USS "Hancock" (CV-19), USS "Bon Homme Richard" (CV-31) and USS "Oriskany" (CV-34) and new construction of a guided missile destroyer, USS "Mahan" (DDG-42). At New York Naval Shipyard (1958... | 11,762 | zeroshot-train |
WASP-1b [SEP] constellation | WASP-1b
WASP-1b is an extrasolar planet orbiting the star WASP-1 located 1,300 light-years away in the constellation Andromeda.
Orbit and mass.
The planet's mass and radius indicate that it is a gas giant with a similar bulk composition to Jupiter. Unlike Jupiter, but similar to many other planets detected around other... | -density planets have been detected by the transit method. In order of discovery they are: HAT-P-1b, COROT-1b, TrES-4, WASP-12b, WASP-17b, and Kepler-7b. Some hot Jupiters detected by the radial-velocity method may be puffy planets. Most of these planets are below two Jupiter masses as more massive planets have stronge... | 11,763 | zeroshot-train |
WASP-6b [SEP] constellation | WASP-6b
WASP-6b is an extrasolar planet approximately 600 light years away in the constellation Aquarius. It was discovered in 2008, by the WASP survey, by astronomical transit across its parent star WASP-6. This planet orbits only 4% that of Earth-Sun distance. The planet has mass half that of Jupiter, but its insolat... | .
WASP-39b is also notable for having an extremely low density, near that of WASP-17b, the least dense known exoplanet. While WASP-17b has a density of g/cm, WASP-39b has a slightly higher density of g/cm.
See also.
- WASP-6b
- WASP-17b
- WASP-19b
- WASP-31b
- WASP-121b | 11,764 | zeroshot-train |
WD 2359-434 [SEP] constellation | WD 2359-434
WD 2359-434 (Gliese 915, LHS 1005, L 362-81) is a nearby degenerate star (white dwarf) of spectral class DAP5.8, the single known component of the system, located in the constellation Phoenix, the nearest star in this constellation.
Distance.
WD 2359-434, probably, is the 11th closest white dwarf, or, possi... | WD 2359-434 is composed of very dense degenerate matter, its mean density is 1,300,000 g·cm, i.e. mass of one cubic millimetre of WD 2359-434 matter is 1.3 kg.
Main sequence progenitor properties.
As all degenerate stars, WD 2359-434 previously existed initially as main-sequence star and then as giant star, until all t... | 11,765 | zeroshot-train |
WISE 0458+6434 [SEP] constellation | WISE 0458+6434
WISEPC J045853.90+643451.9 (designation is abbreviated to WISE 0458+6434) is a binary system of two (A and B) ultracool brown dwarfs of spectral classes T8.5 and T9.5, respectively, located in constellation Camelopardalis at approximately 47 ly from Earth.
History of observations.
History of observations... | of late T-type — T9.5 (initially was estimated as T9).
Distance.
Currently the most accurate distance estimate of WISE 0458+6434 is a trigonometric parallax, measured using Spitzer Space Telescope and published in 2013 by Trent Dupuy and Adam Kraus: 0.070 ± 0.019 arcsec, corresponding to a distance 14.3 pc, or 46.6 ly.... | 11,766 | zeroshot-train |
Wolf 489 [SEP] constellation | Wolf 489
Wolf 489 (WD 1334+039, LHS 46, G 062-053, Gliese 518) is a nearby degenerate star (white dwarf) of spectral class DZ10.0), the single known component of the system, located in the constellation Virgo.
Distance.
Wolf 489, probably, is the 12th closest white dwarf, or, possibly, 9th–14th (see Gliese 293, GJ 1087... | is 121.4 ± 3.4 mas, corresponding to a distance 8.24 ± 0.23 pc, or 26.87 ± 0.75 ly.
Physical parameters.
Wolf 489's mass is 0.55 ± 0.03 Solar masses, its surface gravity is 10 (8.91 · 10) cm·s, or approximately 91 000 of Earth's, corresponding to a radius 9089 km, or 143% of Earth's.
Wolf 489's temperature is 5030 ± 12... | 11,767 | zeroshot-train |
XO-5 [SEP] constellation | XO-5
XO-5 is a yellow dwarf main sequence star located approximately 910 light-years away from Earth in the Lynx constellation. It has a magnitude of about 12 and cannot be seen with the naked eye but is visible through a small telescope.
Planetary system.
The exoplanet XO-5b was discovered by the XO Telescope using th... | XO-1
XO-1 is a magnitude 11 G-type main-sequence star star located approximately 536 light-years away in the constellation Corona Borealis. XO-1 has a mass and radius similar to the Sun.
In 2006 the extrasolar planet XO-1b was discovered orbiting XO-1 by the transit method using the XO Telescope.
Planetary system.
The ... | 11,768 | zeroshot-train |
Xi Tauri [SEP] constellation | Xi Tauri
Xi Tauri (ξ Tau, ξ Tauri) is a hierarchical quadruple system in the constellation Taurus.
Xi Tauri is a spectroscopic and eclipsing quadruple star. It consists of three blue-white B-type main sequence dwarfs. Two of the stars form an eclipsing binary system and revolve around each other once every 7.15 days. T... | -authored over 10 books during his life. He graduated from Huntsville High School and later attending the University of Alabama in Huntsville obtaining a degree in accounting. Record also attended Howard College which today is known as Samford University in Birmingham Alabama. He was later presented with an honorary do... | 11,769 | zeroshot-train |
Zeta Corvi [SEP] constellation | Zeta Corvi
Zeta Corvi, Latinized from ζ Corvi, is a star in the constellation Corvus. It is a blue-white main sequence star of apparent magnitude 5.21. Located around 420 light-years distant, it shines with a luminosity approximately 154 times that of the Sun and has a surface temperature of 10,695 K. It is a Be star, ... | Zeta Crateris
Zeta Crateris (ζ Crateris) is a probable binary star system in the southern constellation of Crater. Zeta Crateris appears to be about half-way between Epsilon Corvi to the southeast and Beta Crateris to the northwest, and marks the lower left corner of the rim of the bowl. Eta Crateris lies somewhat less... | 11,770 | zeroshot-train |
Zeta Equulei [SEP] constellation | 3 Equulei
3 Equulei is a single star located in the small northern constellation of Equuleus. It is faintly visible to the naked eye at an apparent visual magnitude of 5.6. Based upon an annual parallax shift of 4.24 mas, 3 Equulei is roughly distant from Earth, give or take an 80 light-year margin of error. At that di... | " qualifier for the Preakness.
History.
The race was named in honor of famous Italian breeder Federico Tesio, owner of Dormello Stud in Dormelletto, Novara. Tesio was one of the most important breeders of Thoroughbreds in the history of horse racing. His homebreds Nearco and Ribot, both great sires, dominate Thoroughbr... | 11,771 | zeroshot-train |
Zeta Virginis [SEP] constellation | Zeta Virginis
Zeta Virginis (ζ Virginis, abbreviated Zeta Vir, ζ Vir) is a binary star in the zodiac constellation of Virgo. It is visible to the naked eye with an apparent visual magnitude of +3.376 and is located about a half degree south of the celestial equator. Based on parallax measurements obtained during the Hi... | "ζ Virginis" (Latinised to "Zeta Virginis") is the system's Bayer designation. The designations of the two components as "Zeta Virginis A" and "B" derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).
Zeta Virgi... | 11,772 | zeroshot-train |
Zeta Volantis [SEP] constellation | Zeta Volantis
Zeta Volantis (ζ Vol, ζ Volantis) is a binary star system in the southern constellation of Volans. It has an apparent visual magnitude of 3.93, which is bright enough to be seen with the naked eye. Based upon parallax measurements, it is approximately 141 light years from the Sun. The companion is a magni... | the Germans to restore defences that had been removed to allow the evacuation.
On 9 October, the 1st Czechoslovak Armoured Brigade (Major-General Alois Liška) took over the siege. The Czechoslovaks executed frequent raids into the eastern suburbs for nuisance effect and to take prisoners; an attack on 28 October (Czech... | 11,773 | zeroshot-train |
2MASS-GC02 [SEP] constellation | 2MASS-GC02
2MASS-GC02, also known as Hurt 2, is a globular cluster at a distance of about 16 thousand light-years from Earth in the constellation Sagittarius. It was discovered in 2000 by Joselino Vasquez, and confirmed by a team of astronomers under the leadership of R. J. Hurt at 2MASS.
The globular cluster 2MASS-GC0... | Baade's Window is an area with very little obscuring dust that shows objects closer to the Milky Way's center than would normally be visible. NGC 6522, magnitude 8.6, and NGC 6528, magnitude 9.5, are both globular clusters visible through Baade's Window. 20,000 and 24,000 light-years from Earth, with Shapley classes of... | 11,774 | zeroshot-train |
3C 299 [SEP] constellation | 3C 299
3C 299 is a radio galaxy/quasar located in the constellation Boötes.
External links.
- www.jb.man.ac.uk/atlas/ (J. P. Leahy) | , Calif. 29 Sep 1950
- NAS Moffett Field, Calif. 15 Feb 1967
Aircraft Assignment.
The squadron first received the following aircraft on the dates shown:
- PBY-5A May 1946
- PV-2 May 1946
- PBM-5S2 1950
- P5M-1 Jun 1954
- SP-5B 1960
- P-3A Jan 1967
- P-3B Feb 1968
- P-3C Baseline Nov 1971
- P-3C BLOCK MOD Jul 1986
- P-3... | 11,775 | zeroshot-train |
4 Ursae Majoris b [SEP] constellation | 4 Ursae Majoris b
4 Ursae Majoris b (sometimes abbreviated 4 Uma b) is an extrasolar planet orbiting the star 4 Ursae Majoris, approximately 252 light-years away in the constellation of Ursa Major. This planet has a minimum mass over 7 times that of Jupiter and orbits at 0.87 AU from the star in an eccentric path. | Leggatt LJ overturned the High Court, and ICS Ltd appealed.
Judgment.
The House of Lords held by a majority that the right to claim rescission was retained by the investors, but the right to claim for damages had indeed been assigned. Construed in its context, the words ‘Any claim (whether sounding in rescission for un... | 11,776 | zeroshot-train |
53 Aquarii [SEP] constellation | 53 Aquarii
53 Aquarii (abbreviated 53 Aqr) is a binary star system in the equatorial constellation of Aquarius. "53 Aquarii" is its Flamsteed designation though the star also bears the Bayer designation of f Aquarii. The combined apparent visual magnitude of the pair is a 5.56, making it just visible to the naked eye i... | 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... | 11,777 | zeroshot-train |
Antennae Galaxies [SEP] constellation | Antennae Galaxies
The Antennae Galaxies, also known as NGC 4038/NGC 4039, are a pair of interacting galaxies in the constellation Corvus. They are currently going through a starburst phase, in which the collision of clouds of gas and dust, with entangled magnetic fields, causes rapid star formation. They were discovere... | Astronomy Picture of the Day: The Antennae Galaxies (10/22/1997)
- Astronomy Picture of the Day: The Antennae (05/07/2010)
- Astronomy Picture of the Day: The Antennae (04/29/2011)
- Astronomy Picture of the Day: The Antennae (02/12/2015)
- The Register: Galactic prang fingered in star formation mystery
- ESA/Hubble Ne... | 11,778 | zeroshot-train |
Arp 302 [SEP] constellation | Arp 302
Arp 302 (also known as Exclamation Point Galaxy) is a galaxy in the constellation Boötes. Arp 302, also known as VV 340 or UGC 9618 consists of a pair of very gas-rich spiral galaxies in their early stages of interaction. An enormous amount of infrared light is radiated by the gas from massive stars that are fo... | NGC 2857
NGC 2857 (also known as Arp 1 and PGC 26666) is a spiral galaxy in the constellation Ursa Major. It was discovered on January 9, 1856 by R. J. Mitchell.
NGC 2857 is the first object in Halton Arp's Atlas of Peculiar Galaxies, and one of six Arp objects in the 'Low Surface Brightness Galaxies' section. The othe... | 11,779 | zeroshot-train |
Butterfly Cluster [SEP] constellation | Butterfly Cluster
The Butterfly Cluster (cataloged as Messier 6 or M6, and as NGC 6405) is an open cluster of stars in the southern constellation of Scorpius. Its name derives from the vague resemblance of its shape to a butterfly. The Trumpler classification of indicates it is rich in stars (r) with a high concentrati... | - Wizard butterfly, the brush-footed or Bardic wizard butterfly "Rhinopalpa polynice"
- Wizard Nebula, an open cluster located in Cepheus constellation
Sports.
- Wizard (horse) (1806–1813), Thoroughbred racehorse
- Canterbury cricket team, known as the Wizards
- Dakota Wizards, a team in the NBA Development League
- Fo... | 11,780 | zeroshot-train |
COROT-6 [SEP] constellation | COROT-6
COROT-6 is a magnitude 13.9 star located in the Ophiuchus constellation.
Location and properties.
The star has a radius of about 102% of the Sun and a mass of about 110% of the Sun. It is a main sequence F type star a little larger and hotter than the Sun.
Planetary system.
The star is orbited by one known extr... | COROT-1b
COROT-1b (previously named COROT-Exo-1b) is a transiting extrasolar planet approximately 2,630 light-years away in the constellation of Monoceros. The planet was discovered orbiting the yellow dwarf star COROT-1 in May 2007. The planet was the first discovery by the French-led COROT Mission.
Discovery.
COROT-1... | 11,781 | zeroshot-train |
DN Geminorum [SEP] constellation | DN Geminorum
DN Geminorum or Nova Geminorum 1912 was a nova which lit up in 1912 in the constellation Gemini. It reached a brightness of 3.5 mag. Its brightness decreased in 36 days by 3 mag. Today its brightness is 14 mag. | the name for the whole constellation; the name means "Star-wreath" and refers to one of the wives of the Pleiades, called "Makalii".
The stars of Auriga feature in Inuit constellations. Quturjuuk, meaning "collar-bones", was a constellation that included Capella (Alpha Aurigae), Menkalinan (Beta Aurigae), Pollux (Beta ... | 11,782 | zeroshot-train |
Dwingeloo 1 [SEP] constellation | Dwingeloo 1
Dwingeloo 1 is a barred spiral galaxy about 10 million light-years away from the Earth, in the constellation Cassiopeia. It lies in the Zone of Avoidance and is heavily obscured by the Milky Way. The size and mass of Dwingeloo 1 are comparable to those of Triangulum Galaxy.
Dwingeloo 1 has two smaller satel... | Dwingeloo 2
Dwingeloo 2 is a small irregular galaxy discovered in 1996 and located about 10 million light-years away from the Earth. Its discovery was a result of the Dwingeloo Obscured Galaxy Survey (DOGS) of the Zone of Avoidance using the Dwingeloo Radio Observatory. Dwingeloo 2 is a companion galaxy of Dwingeloo 1.... | 11,783 | zeroshot-train |
Eta Scuti [SEP] constellation | Eta Scuti
Eta Scuti (η Sct, η Scuti) is a star in the constellation Scutum.
Eta Scuti is an orange K-type giant with an apparent magnitude of +4.83. It is approximately 202 light years from Earth. This star has 1.4 times the mass of the Sun, more than ten times the Sun's radius, and is about 2.8 billion years old.
Eta ... | GP Andromedae
GP Andromedae (often abbreviated to GP And) is a Delta Scuti variable star in the constellation Andromeda. It is a pulsating star, with its brightness varying with an amplitude of 0.55 magnitudes around a mean magnitude of 10.7.
System.
GP Andromedae is a main sequence Population I star of spectral type A... | 11,784 | zeroshot-train |
GSC 03549-02811 [SEP] constellation | GSC 03549-02811
GSC 03549-02811 (sometimes referred to as TrES-2 A or TrES-2 parent star in reference to its exoplanet TrES-2), also known as Kepler-1) is a yellow main-sequence star similar to our Sun. This star is located approximately 700 light-years away in the constellation of Draco. The apparent magnitude of this... | TrES-2b
TrES-2b (TrES-2 or Kepler-1b) is an extrasolar planet orbiting the star GSC 03549-02811 located 750 light years away from the Solar System. The planet has been identified in 2011 as the darkest known exoplanet, reflecting less than 1% of any light that hits it. The planet's mass and radius indicate that it is a... | 11,785 | zeroshot-train |
Gliese 22 [SEP] constellation | Gliese 22
Gliese 22, also catalogued V547 Cassiopeiae, is a hierarchical star system approximately 33 light-years away in the constellation of Cassiopeia. The system consists of two red dwarf stars, Gliese 22A and Gliese 22B in an outer orbit of about 320 years, and a brown dwarf, Gliese 22C, which orbits Gliese 22A in... | Gliese 163
Gliese 163 is an M3.5V red dwarf located 49 light years (15.0pc) from the sun, in the constellation Dorado. Its coordinates in the night sky are RA 04h 9m 16s and Dec. -53°22'. It has a visual magnitude of 11.8 and an absolute magnitude of 10.9. Other stellar catalog names for it include HIP 19394 and LHS 18... | 11,786 | zeroshot-train |
HAT-P-14b [SEP] constellation | HAT-P-14b
HAT-P-14b is an extrasolar planet located approximately away in the constellation of Hercules, orbiting the 10th magnitude F-type star HAT-P-14. This planet was discovered in 2010 by the HATNet Project using the transit method. It was independently detected by the SuperWASP project.
Orbit.
HAT-P-14b is locate... | is clouded further by the orbital properties of the object: brown dwarfs located close to their stars are rare (a phenomenon known as the brown-dwarf desert), while the majority of the known massive close-in planets (for example XO-3b, HAT-P-2b and WASP-14b) are in highly eccentric orbits, in contrast to the circular o... | 11,787 | zeroshot-train |
HAT-P-9 [SEP] constellation | HAT-P-9
HAT-P-9 is a magnitude 12 F star approximately 1500 light years away in the constellation Auriga. A search for a binary companion star using adaptive optics at the MMT Observatory was negative.
Planetary system.
An exoplanet orbiting the star, HAT-P-9b, was discovered by the transit method on June 26, 2008.
See... | 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 ... | 11,788 | zeroshot-train |
HD 108063 [SEP] constellation | HD 108063
HD 108063 is a star that lies approximately 176 light-years away in the constellation of Centaurus. The star is not particularly noteworthy with exception to its enormously high heavy element content.
Properties.
HD 108063 is a somewhat bright star that lies in an area of the southern sky towards the middle o... | dex).
The enormous metallicity of HD 108063 has strong effect on its apparent parameters. A metal-rich star has a cooler surface temperature than a lower-metallicity star, with the strength of the effect increasing with a higher metallicity. On a plot of B-V (which is an indicator of temperature) to absolute magnitude ... | 11,789 | zeroshot-train |
HD 109749 [SEP] constellation | HD 109749
HD 109749 is a binary star about 206 light years away in the constellation of Centaurus.
Stellar system.
The primary star, HD 109749 A, is a G-type subgiant with a spectral type of G3IV, indicating it is an evolved star with a luminosity higher than that of a main sequence star. It has a mass of and a radius ... | HD 109749 b
HD 109749 b is an extrasolar planet that orbits extremely close to the star HD 109749, taking only 5.24 days to orbit at the distance of 0.063 AU. This planet was discovered on August 22, 2005 - the same day as the discovery of Gliese 581 b.
See also.
- HD 149143 b | 11,790 | zeroshot-train |
HD 1237 [SEP] constellation | HD 1237
HD 1237 is a binary star system approximately 57 light-years away in the constellation of Hydrus (the Water Snake).
The visible star in the system, A, is considered to be a solar analog due close mass to the sun. HD 1237 differs from the sun in that HD 1237 is much younger, has high metallicity, has much cooler... | the Sun, is chromospherically active, and rotates around its axis more quickly than the Sun.
The secondary star was discovered in 2006 during a deep imaging survey conducted at the European Southern Observatory using the Very Large Telescope. HD 1237 B is a M4 red dwarf star at a projected separation of 68 AU.
Planetar... | 11,791 | zeroshot-train |
HD 125823 [SEP] constellation | HD 125823
HD 125823, also known as V761 Centauri or a Centauri, is a star in the constellation Centaurus. It is a blue-white B-type giant with a mean apparent magnitude of +4.41. It is approximately 460 light years from Earth. It is classified as an SX Arietis type variable star and its brightness varies from magnitude... | in 1838). Also called Piazzi's Flying Star, since Giuseppe Piazzi nominated it as a good candidate for distance measurements (parallaxes).
- Bidelman's helium variable star is V761 Centauri (HD 125823). Named after William P. "Billy" Bidelman.
- Bidelman's peculiar star is KS Persei (HD 30353).
- Bidelman's Star is HD ... | 11,792 | zeroshot-train |
HD 135530 [SEP] constellation | HD 135530
HD 135530 is a suspected variable star in the northern constellation of Boötes.
External links.
- HR 5677
- Image HD 135530 | 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-... | 11,793 | zeroshot-train |
HD 143361 [SEP] constellation | HD 143361
HD 143361 is a star in the southern constellation Norma. With an apparent visual magnitude of 9.20, this star is too dim to be seen with the naked eye. It is close enough to the Earth that its distance can be determined using parallax measurements, yielding a value of roughly .
This is a G-type main sequence ... | have a roughly Jupiter-size planet with an orbital period of 2.8 years. HD 143361 is a binary star system composed of a sunlike star and a faint red dwarf separated by 30.9 AU. A planet roughly triple the mass of Jupiter orbits the brighter star every 1057± 20 days. HD 142415 is approximately 113 light-years distant an... | 11,794 | zeroshot-train |
HD 167965 [SEP] constellation | HD 167965
HD 167965 is a 6th magnitude star in the constellation Lyra, approximately 590 light years from Earth. It is a bluish white subgiant star of the spectral type B7IV, meaning it has a surface temperature of 11,000 to 25,000 kelvins. It is larger and brighter than our Sun, and its surface is at least twice as ho... | 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-... | 11,795 | zeroshot-train |
HD 181720 [SEP] constellation | HD 181720
HD 181720 is an 8th magnitude G-type main sequence star located approximately 190 light years away in the constellation Sagittarius. This star is larger, hotter, brighter, and less massive than our Sun. Also its metal content is three-tenths as much as the Sun. In 2009, a gas giant planet was found in orbit a... | HD 5388
HD 5388 (78 G. Phoenicis) is a 7th magnitude F-type main sequence star located approximately 175 light years away in the constellation Phoenix. This star is larger, hotter, brighter, and more massive than our Sun. Also its metal content is half as much as the Sun. In 2009, a gas giant planet was found in orbit ... | 11,796 | zeroshot-train |
HD 195019 [SEP] constellation | HD 195019
HD 195019 (HIP 100970, SAO 106138) is a star system in the constellation of Delphinus. Star B is located approximately 150 AU from Star A. This star system is located away from the Sun, Earth and Solar System. It is a yellow dwarf or subgiant [G3IV-V].
Planetary system.
In 1998, a planet was discovered at Li... | HD 195019 b
HD 195019 b is an exoplanet orbiting around HD 195019 in the binary star system. It has a minimum mass of 3.7 M. It orbits very close to the star. Like many planets at close distance, its orbit is circular, even more circular or less eccentric than Earth. It takes 437 hours to orbit with velocity of 83.24 k... | 11,797 | zeroshot-train |
HD 23089 [SEP] constellation | HD 23089
HD 23089 is a spectroscopic binary star in the northern constellation of Camelopardalis. The system consists of a cooler giant star and hotter main sequence companion, with the pair orbiting each other every 6,150 days.
External links.
- HR 1129
- Image HD 23089 | 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-... | 11,798 | zeroshot-train |
HD 2638 [SEP] constellation | HD 2638
HD 2638 is a dim 10th magnitude star in the constellation of Cetus. It is a yellow dwarf and similar to our Sun. A small telescope is required to view the star. HD 2638 is in a system with multiple stars, including at least HD 2567 and HD 2638 C. HD 2638 is 180 light-years (55 parsecs) from the Sun.
Planetary s... | HD 2638 b
HD 2638 b is a planet of the star HD 2638. It is a typical "hot Jupiter", a planet that orbits its parent star in a very tight "torch orbit". Distance to the star is less than 1/20th Earth's distance from the Sun. One orbital revolution lasts only about three and half days.
External links.
- SIMBAD entry
- Th... | 11,799 | zeroshot-train |
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