query stringlengths 16 148 | pos stringlengths 16 855 | neg stringlengths 0 2.05k | idx int64 0 132k | task_name stringclasses 1
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NGC 2613 [SEP] constellation | NGC 2613
NGC 2613, is a spiral galaxy in the constellation Pyxis. It appears spindle-shaped as it is almost edge-on to observers on Earth. | 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... | 10,900 | zeroshot-train |
NGC 289 [SEP] constellation | NGC 289
NGC 289 is a spiral galaxy in the constellation of Sculptor. The compiler of the New General Catalogue, John Louis Emil Dreyer noted that NGC 289 was "pretty bright, large, extended, between 2 considerably bright stars". It was discovered on September 27, 1834 by John Herschel. | NGC 499
NGC 499, also occasionally referred to as PGC 5060, IC 1686 or GC 289, is a lenticular galaxy in the constellation Pisces. It located approximately 197 million light-years from the Solar System and was discovered on 12 September, 1784 by astronomer William Herschel.
The NGC 499 Group is named after the galaxy.
... | 10,901 | zeroshot-train |
NGC 3281 [SEP] constellation | NGC 3281
NGC 3281 is a large spiral galaxy without a bar in the constellation Antlia. It is a member of the Antlia Cluster, which lies about 98 million light years away. | .
Nearby galaxies.
NGC 3081 is an isolated galaxy. It is located within the same cloud of galaxies with NGC 3223, NGC 3001, NGC 3078, NGC 3089, NGC 3100, NGC 3275, NGC 3281, NGC 3347 and NGC 3449.
See also.
- NGC 6782 - another multiringed galaxy | 10,902 | zeroshot-train |
NGC 3310 [SEP] constellation | NGC 3310
NGC 3310 is a grand design spiral galaxy in the constellation Ursa Major. It is a starburst galaxy and it is likely that NGC 3310 collided with one of its satellite galaxies about 100 million years ago, triggering widespread star formation. It is thought to be located approximately 46 million light-years away ... | structure itself is formed by superwinds from the black hole.
NGC 3310 is another starburst spiral galaxy located 50 million light-years from Earth. Its bright white color is caused by its higher than usual rate of star formation, which began 100 million years ago after a merger. Studies of this and other starburst gal... | 10,903 | zeroshot-train |
NGC 34 [SEP] constellation | NGC 17
NGC 17, also known as NGC 34, is a spiral galaxy in the constellation Cetus. It is the result of a merger between two disk galaxies, resulting in a recent starburst in the central regions and continuing starforming activity. The galaxy is still gas-rich, and has a single galactic nucleus. It lies 250 million lig... | NGC 5866
NGC 5866 (also called the Spindle Galaxy or Messier 102) is a relatively bright lenticular or spiral galaxy in the constellation Draco. NGC 5866 was most likely discovered by Pierre Méchain or Charles Messier in 1781, and independently found by William Herschel in 1788.
Measured orbital velocities of its globu... | 10,904 | zeroshot-train |
NGC 3552 [SEP] constellation | NGC 3552
NGC 3552 is a lenticular galaxy in the constellation Ursa Major. It was discovered in April 1785 by William Herschel. | 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... | 10,905 | zeroshot-train |
NGC 3766 [SEP] constellation | NGC 3766
NGC 3766 is an open star cluster in the southern constellation Centaurus. It is located in the vast star-forming region known as the Carina molecular cloud, and was discovered by Nicolas Louis de Lacaille during his astrometric survey in 1751–1752. At a distance of about 1745 pc, the cluster subtends a diamete... | cooler than slowly pulsating B stars.
See also.
- New General Catalogue
External links.
- NGC 3766 at SEDS
- Astrophotograph Link
- WEBDA Data on NGC 3766 by Lynga | 10,906 | zeroshot-train |
NGC 4013 [SEP] constellation | NGC 4013
NGC 4013 is an edge-on barred spiral galaxy about 55 million light-years away in the constellation Ursa Major. The disk of NGC 4013 shows a distinct "peanut"-shaped bulge in long exposure photographs that N-body computer simulations suggest is consistent with a stellar bar seen perpendicular to the line of sig... | 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) | 10,907 | zeroshot-train |
NGC 4036 [SEP] constellation | NGC 4036
NGC 4036 is the "New General Catalogue" identifier for a lenticular galaxy in the northern circumpolar constellation of Ursa Major. In the "Carnegie Atlas of Galaxies", it is described as being "characterized by an irregular
pattern of dust lanes threaded through the disc in an 'embryonic' spiral pattern indic... | NGC 7302
NGC 7302 is a lenticular galaxy located around 124 million light-years away from Earth in the constellation of Aquarius. NGC 7302 was discovered by British astronomer William Herschel on October 3, 1785 and was rediscovered by American astronomer Lewis Swift on August 8, 1896 and was listed in the IC catalogue... | 10,908 | zeroshot-train |
NGC 4550 [SEP] constellation | NGC 4550
NGC 4550 is a barred lenticular galaxy located in the constellation of Virgo that can be seen with amateur telescopes. It lies at a distance of 50 million light-years (15.5 mega parsecs) from the Milky Way and is a member of the Virgo Cluster.
Physical characteristics.
While NGC 4550 is not one of the brightes... | is the spiral galaxy NGC 7217. The stars of this galaxy are concentrated in two disks of similar size and surface brightness, one nested within the other and it has been suggested it's the product of the merger between two previous disk galaxies, each one counter-rotating with respect to the other.
NGC 4550's center al... | 10,909 | zeroshot-train |
NGC 4625 [SEP] constellation | NGC 4625
NGC 4625 is a distorted dwarf galaxy in the constellation Canes Venatici. The galaxy is formally classified as a Sm galaxy, which means that its structure vaguely resembles the structure of spiral galaxies. The galaxy is sometimes referred to as a Magellanic spiral because of its resemblance to the Magellanic ... | NGC 5398
NGC 5398 is a barred spiral galaxy in the constellation Centaurus.
See also.
- NGC 4618 - "a similar galaxy"
- NGC 4625 - "a similar galaxy"
External links.
- GALEX page on NGC 5398 | 10,910 | zeroshot-train |
NGC 4634 [SEP] constellation | NGC 4634
NGC 4634 is an edge-on barred spiral galaxy located about 70 million light-years away in the constellation of Coma Berenices. NGC 4634 was discovered by astronomer William Herschel on January 14, 1787. It is interacting with the spiral galaxy NGC 4633. Both galaxies are members 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... | 10,911 | zeroshot-train |
NGC 4780 [SEP] constellation | NGC 4780
NGC 4780 is an intermediate spiral galaxy within the constellation Virgo. | 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... | 10,912 | zeroshot-train |
NGC 5253 [SEP] constellation | NGC 5253
NGC 5253 is an irregular galaxy in the constellation Centaurus. It was discovered by William Herschel on 15 March 1787.
Properties.
NGC 5253 is located within the M83 Subgroup of the Centaurus A/M83 Group, a relatively nearby galaxy group that includes the radio galaxy Centaurus A and the spiral galaxy M83 (th... | Self Published version.
External links.
- Light curves and spectra on the Open Supernova Catalog
- First images (1972). Photo comparisons of NGC 5253 in June 1959 then in May 1972 showing first images of the actual SN 1972e explosion near NGC 5253 (Palomar Observatory blog).
- SIMBAD, SN 1972E
- SN 1972E in NGC 5253 De... | 10,913 | zeroshot-train |
NGC 5754 [SEP] constellation | NGC 5754
NGC 5754 is a barred spiral galaxy located 218 million light years away in the constellation Boötes. It is a member of the Arp 297 interacting galaxies group, which consists of NGC 5752, NGC 5753, NGC 5754, NGC 5755. Along with NGC 2718 and UGC 12158, NGC 5754 is often considered a Milky Way-twin.
External lin... | 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... | 10,914 | zeroshot-train |
NGC 5879 [SEP] constellation | NGC 5879
NGC 5879 is a spiral galaxy in the constellation Draco. The galaxy was discovered in 1788 by William Herschel. It is a member of the NGC 5866 Group. | corresponding objects.
Although M101 and NGC 5866 are considered to be the two most likely candidates for M102, a few other objects have been suggested as potentially corresponding to this entry.
Candidate corresponding objects Other possible corresponding objects NGC 5879, NGC 5907, NGC 5908.
NGC 5879, NGC 5907, NGC 5... | 10,915 | zeroshot-train |
NGC 5986 [SEP] constellation | NGC 5986
NGC 5986 is a globular cluster in the constellation Lupus. | magnitude every 7 hours and 6 minutes.
Features Deep-sky objects.
Towards the north of the constellation are globular clusters NGC 5824 and NGC 5986, and close by the dark nebula B 228. To the south are two open clusters, NGC 5822 and NGC 5749, as well as globular cluster NGC 5927 on the eastern border with Norma. On t... | 10,916 | zeroshot-train |
NGC 6167 [SEP] constellation | NGC 6167
NGC 6167 is an open cluster in the constellation of Norma, viewed from Earth it has an apparent magnitude of 6.7. | 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... | 10,917 | zeroshot-train |
NGC 6207 [SEP] constellation | NGC 6207
NGC 6207 is a spiral galaxy located in the constellation Hercules. It is designated as SA(s)c in the galaxy morphological classification scheme and was discovered by William Herschel on 16 May 1787. NGC 6207 is located at about 30 million light years from earth. It is located near the globular cluster Messier ... | summer.
It is located at right ascension 16 41.7, declination +36° 28'. With an apparent magnitude of 5.8, it is barely visible with the naked eye on clear nights. Its diameter is about 23 arc minutes and it is readily viewable in small telescopes. Nearby is NGC 6207, a 12th magnitude edge-on galaxy that lies 28 arc mi... | 10,918 | zeroshot-train |
NGC 625 [SEP] constellation | NGC 625
NGC 625 is a dwarf barred spiral galaxy about 12.7 Mly away in the constellation Phoenix. NGC 625 is a member of the Sculptor Group. | Sun has and hence must have formed very early in the history of the universe. With a visual magnitude of 15.17, it is around 10,000 times dimmer than the faintest stars visible to the naked eye and is 36000 light years distant.
Features Deep-sky objects.
The constellation does not lie on the galactic plane of the Milky... | 10,919 | zeroshot-train |
NGC 6251 [SEP] constellation | NGC 6251
NGC 6251 is an active supergiant elliptical radio galaxy in the constellation Ursa Minor, and is more than 340 million light-years away from Earth. The galaxy has a Seyfert 2 active galactic nucleus, and is one of the most extreme examples of a Seyfert galaxy. This galaxy may be associated with gamma-ray sourc... | . The supermassive black hole at the core has a mass of .
External links.
- www.jb.man.ac.uk/atlas/
- Wikisky image of NGC 6251
- Hubble Finds a Bare Black Hole Pouring Out Light (Probing the heart of the active galaxy NGC 6251—September 10, 1997) | 10,920 | zeroshot-train |
NGC 637 [SEP] constellation | NGC 637
NGC 637 is an open cluster of stars in the constellation Cassiopeia. It has a Trumpler classification of I2m and an angular diameter of 4.2′. At a distance of approximately 7,045 light years, this corresponds to a diameter of . The estimated age of this cluster is 5–15 million years.
The cluster was discovered ... | 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... | 10,921 | zeroshot-train |
NGC 6380 [SEP] constellation | NGC 6380
NGC 6380 is a globular cluster located in the constellation Scorpius. It was discovered by the British astronomer John Herschel on 29 June 1834. It is at a distance of about 35,500 light years away from earth. NGC 6380 was initially characterized as an open cluster, and given the designation Pişmiş 25, however... | 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... | 10,922 | zeroshot-train |
NGC 6541 [SEP] constellation | NGC 6541
NGC 6541 (also known as Caldwell 78) is a globular cluster in the southern constellation of Corona Australis. It is estimated to be around 14 billion years old.
The globular cluster was discovered by Niccolò Cacciatore at the Palermo Astronomical Observatory, Sicily, on March 19, 1826. It was independently fou... | open cluster ESO 281-SC24, which is composed of the yellow 9th magnitude star GSC 7914 178 1 and five 10th to 11th magnitude stars. Halfway between Theta Coronae Australis and Theta Scorpii is the dense globular cluster NGC 6541. Described as between magnitude 6.3 and magnitude 6.6, it is visible in binoculars and smal... | 10,923 | zeroshot-train |
NGC 6584 [SEP] constellation | NGC 6584
NGC 6584 is a globular cluster in the constellation Telescopium that lies near Theta Arae and is 45000 light-years distant. It is an Oosterhoff type I cluster, and contains at least 69 variable stars, most of which are RR Lyrae variables: 46 stars were identified as RRab variables, 15 as RRc variables, 1 RRe v... | instrument on the ESO 3.6 m Telescope, it was found to have a brown dwarf around 38 times as massive as Jupiter orbiting at an average distance of 1.35 AU with a period of 505 days. This is an unusually close distance from the star, within a range that has been termed the brown-dwarf desert.
Features Deep sky objects.
... | 10,924 | zeroshot-train |
NGC 6760 [SEP] constellation | NGC 6760
NGC 6760 is a globular cluster in the constellation Aquila.
External links.
- Simbad
- NGC 6760 | 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... | 10,925 | zeroshot-train |
NGC 6811 [SEP] constellation | NGC 6811
NGC 6811 is an open cluster in the constellation of Cygnus, near the constellation of Lyra. It has an angular size half that of the full Moon and includes about 1000 stars of roughly similar magnitude. It has also been called "The Hole in the Cluster" because of its dark center.
Features.
NGC 6811 lies far awa... | variables are too old to be associated with open clusters, and are instead found in globular clusters.
Planets.
The open cluster NGC 6811 contains two known planetary systems Kepler 66 and Kepler 67.
See also.
- List of open clusters
- Moving groups
- Open cluster family
- Open cluster remnant
External links.
- The Jew... | 10,926 | zeroshot-train |
NGC 75 [SEP] constellation | NGC 75
NGC 75 is a lenticular galaxy estimated to be about 260 million light-years away in the constellation of Pisces. It was discovered by Lewis A. Swift from the USA in 1886 and its magnitude is 13.2. | NGC 4429
NGC 4429 is a lenticular galaxy located about 55 million light-years away in the constellation of Virgo. NGC 4429 is tilted at an inclination of about 75° which means that the galaxy is tilted almost edge-on as seen from Earth. NGC 4429 was discovered by astronomer William Herschel on March 15, 1784. The galax... | 10,927 | zeroshot-train |
NGC 7510 [SEP] constellation | NGC 7510
NGC 7510 is an open cluster of stars located around 11,400 light years away in the constellation Cepheus, near the border with Cassiopeia. At this distance, the light from the cluster has undergone extinction from interstellar gas and dust equal to = magnitude in the UBV photometric system. Its brightest membe... | 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... | 10,928 | zeroshot-train |
NGC 76 [SEP] constellation | NGC 76
NGC 76 is a lenticular galaxy estimated to be about 325 million light-years away in the constellation of Andromeda. It was discovered by Guillaume Bigourdan from France in 1884 and its magnitude is 13.1. | NGC 191A
NGC 191A (also PGC 2332, IC 1563, MCG -2-2-76 of ARP 127) is a lenticular galaxy in the constellation Cetus.
See also.
- List of NGC objects | 10,929 | zeroshot-train |
NGC 98 [SEP] constellation | NGC 98
NGC 98 is a barred spiral galaxy in the Phoenix constellation. The galaxy NGC 98 was discovered on September 6, 1834 by the British astronomer John Frederick William Herschel.
External links.
- SEDS | 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 ... | 10,930 | zeroshot-train |
Nu Centauri [SEP] constellation | Nu Centauri
Nu Centauri (ν Cen, ν Centauri) is a binary star system in the southern constellation of Centaurus. The combined apparent visual magnitude of the pair is +3.41, making this one of the brightest members of the constellation. Based upon parallax measurements made during the Hipparcos mission, this star system... | Domino, Jay Biz
- scratching – Touré
- vocals – A+, Del tha Funkee Homosapien, Extra Prolific, Pep Love, Phesto, Souls of Mischief, Tajai | 10,931 | zeroshot-train |
OGLE-2007-BLG-368Lb [SEP] constellation | OGLE-2007-BLG-368Lb
OGLE-2007-BLG-368Lb is an extrasolar planet located approximately 19,230 light-years away in the constellation of Scorpius, orbiting the star OGLE-2007-BLG-368L. This planet was detected on December 8, 2009 by the gravitational microlensing by Sumi. It has mass 6.94% of Jupiter (i.e. 22 times that o... | the Automated Robotic Terrestrial Exoplanet Microlensing Search (ARTEMiS). RoboNet-II aims at obtaining a first census of cool terrestrial exoplanets.
Research highlights.
RoboNet data have contributed to the detection of several extra-solar planets (in the order of announcement of their discovery)
- OGLE-2005-BLG-071L... | 10,932 | zeroshot-train |
Palomar 1 [SEP] constellation | Palomar 1
Palomar 1 is a globular cluster in the constellation Cepheus in the
halo possibly in the Outer Arm of the Milky Way galaxy. First discovered by George O. Abell in 1954 on the Palomar Survey Sky plates,
it was catalogued as a globular cluster. At 6.3 to 8 Gyr, it is a very young cluster when compared to the ot... | Lyman-alpha blob 1
Lyman-alpha blob 1 (LAB-1) is a giant cosmic cloud of gas located at the southern constellation of Aquarius, approximately 11.5 billion light-years from Earth with a redshift (z) of 3.09. It was discovered unexpectedly in 2000 by Charles Steidel and colleagues, who were surveying for high-redshift ga... | 10,933 | zeroshot-train |
Palomar 2 [SEP] constellation | Palomar 2
Palomar 2 is a globular cluster located in the constellation of Auriga. Palomar 2 is part of a group of 15 globulars known as the Palomar clusters, discovered in survey plates from the first National Geographic Society – Palomar Observatory Sky Survey in the 1950s. | -up observations were conducted by the High Resolution Echelle Spectrometer at the W.M. Keck Observatory in Hawaii, as well as the WIYN Observatory in Arizona and the Palomar Observatory in California.
Host star.
Kepler-9 is a sun-like star in the constellation Lyra that lies some 640 parsecs away from Earth. With a ma... | 10,934 | zeroshot-train |
Pi Aquarii [SEP] constellation | Pi Aquarii
Pi Aquarii, Latinized from π Aquarii, is the Bayer designation for a binary star in the equatorial constellation of Aquarius. This system has an apparent visual magnitude of a mean apparent magnitude of +4.57. Based upon parallax measurements, it is located at a distance of roughly from Earth.
This is a bina... | and its brightness varies from magnitude +4.45 to +4.71; a range of 0.28. The dominant variability period, , is nearly the same as the orbital period. Pi Aquarii has a reasonable chance of becoming a supernova some day.
In culture.
Pi Aquarii was called "Seat" by Grotius in the 17th century, but the name has rarely bee... | 10,935 | zeroshot-train |
Pi Cephei [SEP] constellation | Pi Cephei
Pi Cephei (π Cephei) is a trinary star located in the constellation Cepheus. With a combined apparent magnitude of about 4.4, the system is faintly visible to the naked eye. The inner pair of stars orbits in 1.5 years while the outer companion completes one orbit in about 160 years.
Stellar system.
Pi Cephei ... | has been exhausted, they are enlarging and cooling to eventually become red giant stars. Markab has an apparent magnitude of 2.48, while Algenib is a Beta Cephei variable that varies between magnitudes 2.82 and 2.86 every 3 hours 38 minutes, and also exhibits some slow pulsations every 1.47 days.
Eta and Omicron Pegasi... | 10,936 | zeroshot-train |
Pi Herculis [SEP] constellation | Pi Herculis
Pi Herculis (π Her, π Herculis) is a third-magnitude star in the constellation Hercules. As one of the four stars in the Keystone asterism (see yellow quadrangle), it is one of the constellation's more easily recognized. It has an apparent visual magnitude of +3.2, which is visible to the naked eye and make... | Pi as two stars each. Nu is also the same star as Psi Herculis. John Flamsteed numbered 54 stars for the constellation.
Located 36.7 light-years from Earth, Arcturus, or Alpha Boötis, is the brightest star in Boötes and the fourth-brightest star in the sky at an apparent magnitude of −0.05; It is also the brightest sta... | 10,937 | zeroshot-train |
RR Telescopii [SEP] constellation | RR Telescopii
RR Telescopii is a symbiotic nova in the southern constellation Telescopium. It was recorded on photographic survey plates as a faint variable star between photographic magnitude (m) 9 to 16.6 from 1889 to 1944. In late 1944 the star began to brighten, increasing by about 7 magnitudes, from m ≈ 14 to brig... | white dwarf.
While RR Telescopii, also designated "Nova Telescopii 1948", is often called a slow nova, it is now classified as a symbiotic nova system composed of an M5III pulsating red giant and a white dwarf; between 1944 and 1948 it brightened by about 7 magnitudes before being noticed at apparent magnitude 6.0 in m... | 10,938 | zeroshot-train |
Rho Ophiuchi [SEP] constellation | Rho Ophiuchi
Rho Ophiuchi (ρ Ophiuchi) is a multiple star system in the constellation Ophiuchus. The central system has an apparent magnitude of 4.63. Based on the central system's parallax of 9.03 mas, it is located about 360 light-years (110 parsecs) away. The other stars in the system are slightly farther away.
Syst... | Omicron Scorpii
Omicron Scorpii (ο Sco, ο Scorpii) is a star in the zodiac constellation of Scorpius. With an apparent visual magnitude of +4.57, it is visible to the naked eye. Parallax measurements indicate a distance of roughly 900 light years. It is located in the proximity of the Rho Ophiuchi dark cloud.
This is a... | 10,939 | zeroshot-train |
Ross 614 [SEP] constellation | Ross 614
Ross 614 (V577 Monocerotis) is a red dwarf UV Ceti flare star and it is the primary member of a nearby binary star system in the constellation of Monoceros. This star has a magnitude of about 11, making it invisible to the unaided eye even though it is one of the stars nearest to the Sun. This system is among ... | facility still within the 14th Air Force HQ building. The 1st Space Control Squadron became part of the 614 AOC / JSpOC.
21 Sep 2007 The ribbon is cut on a new operations center which consolidated all 614 AOC units at Vandenberg Air Force Base in California. Operations began in the new facility on 18 Aug 2007. General ... | 10,940 | zeroshot-train |
SN 2002bj [SEP] constellation | SN 2002bj
SN 2002bj was the explosion of a star in the galaxy NGC 1821, located in the constellation
Lepus. The explosion was discovered by Jack Newton in scans of images produced by Tim Puckett. (It was independently discovered by the Lick/Tenagra Observatory as part of their combined supernova search program.) Initia... | with modern data on typical supernovae of Type Ia; so SN 1885A had been assigned to this type. Recent studies led by Dovi Poznanski and by Hagai Perets suggest that SN 1885A belongs in a new subclass of Type I supernovae along with SN 2002bj and SN 1939B.
The location of the supernova event was 16″ from the relatively ... | 10,941 | zeroshot-train |
Saturn Nebula [SEP] constellation | Saturn Nebula
The Saturn Nebula or NGC 7009 is a planetary nebula in the constellation Aquarius. It appears as a greenish-yellowish hue in a small amateur telescope. It was discovered by William Herschel on September 7, 1782, using a telescope of his own design in the garden at his home in Datchet, England, and was one... | C55
C55 or C-55 can refer to:
- JNR Class C55, a Japanese steam locomotive type
- C-55 Commando, a World War II transport aircraft
- "Corydoras xinguensis", the Xingu corydoras, a freshwater catfish code
- Shipowners' Liability (Sick and Injured Seamen) Convention, 1936 code
- a C serie model of Wordtank Japanese elect... | 10,942 | zeroshot-train |
Sigma Geminorum [SEP] constellation | Sigma Geminorum
Sigma Geminorum (σ Gem) is a binary star system in the constellation Gemini, just to the northeast of Pollux. It is visible to the naked eye with an apparent visual magnitude of 4.20. Based upon an annual parallax shift of 26.08 mas, it is located 125 light years from the Sun.
Sigma Geminorum is a singl... | 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 ... | 10,943 | zeroshot-train |
T Tauri [SEP] constellation | T Tauri
T Tauri is a variable star in the constellation Taurus, the prototype of the T Tauri stars. It was discovered in October 1852 by John Russell Hind. T Tauri appears from Earth amongst the Hyades cluster, not far from ε Tauri; but it is actually 420 light years behind it and was not formed with the rest of them. ... | PDS 110
PDS 110 is a young 11th magnitude star located approximately away in the constellation Orion. In 2017, it was discovered that the star is orbited by an exoplanet or brown dwarf with a disk of dust around it.
Description.
PDS 110 is a young star still approaching the main sequence. It has been classified as a T ... | 10,944 | zeroshot-train |
TX Piscium [SEP] constellation | TX Piscium
TX Piscium (19 Piscium) is a variable carbon star in the constellation Pisces. It is amongst the reddest naked eye stars, with a significant reddish hue when seen in binoculars. It is approximately 900 light years from Earth.
Spectrum.
TX Piscium is a very red star, 2.6 magnitudes fainter at blue wavelengths... | several TDUs, the abundance of carbon in the atmosphere begins to exceed that of oxygen and then the star is known as a carbon star. In TX Piscium, the carbon/oxygen ratio is calculated to be 1.03, which is at the low end of the scale of carbon stars. It is thought to be a relatively new carbon star.
TX Piscium has a m... | 10,945 | zeroshot-train |
Theta Apodis [SEP] constellation | Theta Apodis
Theta Apodis (θ Aps, θ Apodis) is the Bayer designation for a star in the southern circumpolar constellation of Apus. It is a variable star with an apparent visual magnitude range of 4.65 to 6.20, which, according to the Bortle Dark-Sky Scale, means it is a faint star but visible to the naked eye from dark... | of times the mass of the Sun per year through its stellar wind. Dusty material ejected from this star is interacting with the surrounding interstellar medium, forming a bow shock as the star moves through the galaxy. The stand-off distance for this front is located at about from Theta Apodis.
Theta Apodis has been iden... | 10,946 | zeroshot-train |
Theta Tauri [SEP] constellation | Theta Tauri
Theta Tauri (θ Tauri, abbreviated Theta Tau, θ Tau) is a wide double star in the constellation of Taurus and a member of the Hyades open cluster.
θ Tauri is composed of two 3rd magnitude stars, designated Theta¹ Tauri (Theta Tauri B) and Theta² Tauri (Theta Tauri A). Theta² is brighter, hence the pair are s... | between 27.9° and 56.2° in the equatorial coordinate system.
History and mythology In non-Western astronomy.
The stars of Auriga were incorporated into several Chinese constellations. "Wuche", the five chariots of the celestial emperors and the representation of the grain harvest, was a constellation formed by Alpha Au... | 10,947 | zeroshot-train |
V4199 Sagittarii [SEP] constellation | V4199 Sagittarii
V4199 Sagittarii is a star in the constellation Sagittarius. It is a slowly pulsating B star that varies between apparent magnitudes
6.22 and 6.28 over a period of 1.23825 days. | with Grace, and returned to solo work as well as collaborating with Tilt. She also was the vocalist in Elevate feat Dominique on "Next Life"; and Mekka's "Diamondback". In 1999 she performed vocals, mixed with those of Patti Low, in Grace's re-release of "Not Over Yet". Atkins also appeared in Grace music videos as the... | 10,948 | zeroshot-train |
WASP-19 [SEP] constellation | WASP-19
WASP-19 is a magnitude 12.3 star located in the Vela constellation of the southern hemisphere. This star has been found to host a transiting hot Jupiter-type planet in tight orbit.
Planetary system.
In December 2009 SuperWASP project announced that a hot Jupiter type extrasolar planet, WASP-19b, was orbiting ve... | 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... | 10,949 | zeroshot-train |
WASP-43 [SEP] constellation | WASP-43
WASP-43 is a K-type star in the Sextans constellation. It is about half the size of the Sun, and has approximately half the mass. WASP-43 has one known planet in orbit, a Hot Jupiter called WASP-43b. At the time of publishing of WASP-43b's discovery on April 15, 2011, the planet was the most closely orbiting Ho... | Midway.
- Enterprise Air Group Established 1 July 1938 to fly from USS Enterprise (CV-6), disestablished 1 Sep 1942 after USS Enterprise was damaged during the Battle of the Eastern Solomons and entered Pearl Harbor naval shipyard for repairs.
- Wasp Air Group Established 1 Jul 1939 to fly from USS Wasp (CV-7), disesta... | 10,950 | zeroshot-train |
WR 22 [SEP] constellation | WR 22
WR 22, also known as V429 Carinae or HR 4188, is an eclipsing binary star system in the constellation Carina. The system contains a Wolf-Rayet (WR) star that is one of the most massive and most luminous stars known, and is also a bright x-ray source due to colliding winds with a less massive O class companion.
Sy... | HD 151932
HD 151932, also known as WR 78, is a Wolf-Rayet star located in the constellation Scorpius, close to the galactic plane. Its distance is around 1,300 parsecs (4,200 lightyears) away from the Earth. Despite being a blue-colored Wolf-Rayet star, it is extremely reddened by interstellar extinction, so its appare... | 10,951 | zeroshot-train |
XO-5b [SEP] constellation | XO-5b
XO-5b is an extrasolar planet approximately 910 light years away in the constellation of Lynx. This planet was found by the transit method using the XO Telescope and announced in May 2008. It was also independently discovered by the HATNet Project. The planet has a mass and radius just slightly larger than that o... | summit of the Haleakalā volcano in Hawaii. Their first discovery of a Jupiter-sized planet orbiting a Sun-like star 600 light-years from Earth in the constellation Corona Borealis—XO-1b—was reported May 16, 2006 on Newswise.
In 2016 three similar double telescopes were operating, two in Spain and one in Utah.
Discoveri... | 10,952 | zeroshot-train |
YZ Ceti [SEP] constellation | YZ Ceti
YZ Ceti is a red dwarf star in the constellation Cetus. Although it is relatively close to the Sun at just 12 light years, this star cannot be seen with the naked eye. It is classified as a flare star that undergoes intermittent fluctuations in luminosity. YZ Ceti is about 13 percent the mass of the Sun and 17%... | longer orbital period of YZ Ceti b of 2.02 days rather than 1.97 days, and additionally finding that YZ Ceti c probably orbits in only 0.75 days rather than 3.06 days. If the latter is true, YZ Ceti c would have a mass of only 0.58 Earth masses and a roughly 10% chance of transiting YZ Ceti.
See also.
- List of nearest... | 10,953 | zeroshot-train |
Zeta Persei [SEP] constellation | Zeta Persei
Zeta Persei (ζ Per, ζ Persei) is a star in the northern constellation of Perseus. With an apparent visual magnitude of 2.9, it can be readily seen with the naked eye. Parallax measurements place it at a distance of about from Earth.
Description.
This is a lower luminosity supergiant star with a stellar clas... | been considered a member of the group, but is actually located a mere 34 light-years distant. This star is very similar to our Sun, shining with 2.2 times its luminosity. It is a yellow main sequence star of spectral type G0V. Extensive searches have failed to find evidence of it having a planetary system.
Zeta Persei ... | 10,954 | zeroshot-train |
10 Aquarii [SEP] constellation | 10 Aquarii
10 Aquarii (abbreviated 10 Aqr) is a A-type main-sequence star in the constellation of Aquarius. "10 Aquarii" is the Flamsteed designation. It is approximately 400 ly from Earth, based on parallax. | 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... | 10,955 | zeroshot-train |
110 Virginis [SEP] constellation | 110 Virginis
110 Virginis is a star in the zodiac constellation Virgo, located 195 light years away from the Sun. It is visible to the naked eye as an orange-hued star with an apparent visual magnitude of 4.40. The star is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.
The stellar classific... | 101 Virginis
101 Virginis is a red giant variable star in the Boötes constellation, currently on the asymptotic giant branch. It was originally catalogued as 101 Virginis by Flamsteed due to an error in the position. When it was confirmed as a variable star, it was actually within the border of the constellation Bootes... | 10,956 | zeroshot-train |
16 Cephei [SEP] constellation | 16 Cephei
16 Cephei is a single star located about 119 light years away from the Sun in the constellation of Cepheus. It is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of 5.036. The star has a relatively high proper motion, traversing the celestial sphere at the rate of... | "Enoclerus erro"
- "Enoclerus erwini"
- "Enoclerus eximius"
- "Enoclerus fasciicollis"
- "Enoclerus festivus"
- "Enoclerus fibrillatus"
- "Enoclerus franki"
- "Enoclerus fugitivus"
- "Enoclerus gabriellae"
- "Enoclerus gerhardi"
- "Enoclerus gibbus"
- "Enoclerus gilli"
- "Enoclerus gumae"
- "Enoclerus hespenheidei"
- "... | 10,957 | zeroshot-train |
36 Ursae Majoris [SEP] constellation | 36 Ursae Majoris
36 Ursae Majoris is a double star in the northern constellation of Ursa Major. With an apparent visual magnitude of 4.82, it can be seen with the naked eye in suitable dark skies. Based upon parallax measurements, this star lies at a distance of from Earth.
This star is a solar analog—meaning it has ph... | 20 February 1946
- 380th Bombardment Group, 17 July 1947 – 27 June 1949
- 380th Bombardment Wing, 11 July 1955 – 25 June 1966, 6 January 1971 – 30 September 1995
History Stations.
- Davis-Monthan Field, Arizona, 3 November 1942
- Biggs Field, Texas, 2 December 1942
- Lowry Field, Colorado, 4 March-19 Apx 1943
- Manbull... | 10,958 | zeroshot-train |
3C 171 [SEP] constellation | 3C 171
3C 171 is a Seyfert galaxy located in the constellation Lynx.
External links.
- www.jb.man.ac.uk/atlas/ | , 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... | 10,959 | zeroshot-train |
3C 191 [SEP] constellation | 3C 191
3C 191 is a quasar located in the constellation Cancer. | , 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... | 10,960 | zeroshot-train |
3C 215 [SEP] constellation | 3C 215
3C 215 is a Seyfert galaxy / Quasar located in the constellation Cancer.
External links.
- www.jb.man.ac.uk/atlas/ | , 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... | 10,961 | zeroshot-train |
3C 249.1 [SEP] constellation | 3C 249.1
3C 249.1 is a Seyfert galaxy located in the constellation Draco.
External links.
- www.jb.man.ac.uk/atlas/
- Simbad | , 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... | 10,962 | zeroshot-train |
3C 305 [SEP] constellation | 3C 305
3C 305 is a Seyfert 2 radio galaxy located in the constellation Draco. | , 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... | 10,963 | zeroshot-train |
49 Arietis [SEP] constellation | 49 Arietis
49 Arietis is a single star in the northern constellation of Aries. "49 Arietis" is the Flamsteed designation. It is visible to the naked eye as a faint, white hued star with an apparent visual magnitude of 5.90. The star is located at a distance of about distant from Earth based on parallax.
This object is ... | labor costs. Thus, the zone largely determined the location and success of the original movie ranches in or near Hollywood. By establishing movie ranches around the periphery of the zone, studios could take advantage of Los Angeles's varied landscape. With clever editing, it was easy to use a few aerial and location sh... | 10,964 | zeroshot-train |
54 Ceti [SEP] constellation | 54 Ceti
54 Ceti is an older Flamsteed designation for a star that is now located within the constellation boundaries of Aries, the Ram. In the present day it is known by star catalogue identifiers like "HD 11257" or "HR 534". At an apparent visual magnitude of 5.94, it can be seen with the naked eye. The distance to th... | Beta Ceti
Beta Ceti (β Ceti, abbreviated Beta Cet, β Cet), also named Diphda , is the brightest star in the constellation of Cetus. Although designated 'beta', it is actually brighter than the 'alpha' star in the constellation (Alpha Ceti). This orange giant is easy to identify due to its location in an otherwise dark ... | 10,965 | zeroshot-train |
70 Virginis b [SEP] constellation | 70 Virginis b
70 Virginis b (abbreviated 70 Vir b) is an extrasolar planet approximately 60 light-years away in the constellation of Virgo. Announced in 1996 by Geoffrey Marcy and R. Paul Butler, 70 Virginis was one of the first stars confirmed to have planets orbiting it. When first announced, 70 Virginis b was consid... | External links.
- Official site | 10,966 | zeroshot-train |
AN Ursae Majoris [SEP] constellation | AN Ursae Majoris
AN Ursae Majoris is a variable star in the constellation Ursa Major. This star has the strongest known magnetic field among cataclysmic variables, with a field strength of 230 million gauss (23 kT). This object, along with AM Herculis, define a class of objects known as "polars". | , being both a Site of Special Scientific Interest (SSSI) and a Special Area of Conservation (SAC): these designations cover a wider area than the NNR ("c". 11.5 km). Moine Mhòr lies within the Knapdale national scenic area (NSA)
External links.
- Moine Mhòr National Nature Reserve - Scottish Natural Heritage
- Scotlan... | 10,967 | zeroshot-train |
AT Microscopii [SEP] constellation | AT Microscopii
AT Microscopii is a binary star system located at a distance of from the Sun in the constellation of Microscopium. Both members are flare stars, meaning they are red dwarf stars that undergo random eruptions that increase their brightness. This pair lies physically near the red dwarf star AU Microscopii,... | Manual of the Soviet Politburger, (2001) Agent Orange, the feature film The Subversion Agency (2004) and the documentary "60 Seconds of Solitude in Year Zero".
For many years Boswell has taught at the San Francisco Art Institute, The Ringling College of Art and Design, Florida, and the Pratt Institute in New York. He w... | 10,968 | zeroshot-train |
BO Microscopii [SEP] constellation | BO Microscopii
BO Microscopii (BO Mic) is a star in the constellation Microscopium located about from the Sun. It has been dubbed "Speedy Mic" because of its very rapid rotation. The projected rotational velocity at the equator of this star is about , which, with an estimated inclination of 70° to the line of sight fro... | 8 light-years distant. It passed within 1.14 and 3.45 light-years of the Sun some 3.9 million years ago, possibly disturbing the outer Solar System. Two star systems—WASP-7 and HD 205739—have been determined to have planets, while two others—the young red dwarf star AU Microscopii and the sunlike HD 202628—have debris ... | 10,969 | zeroshot-train |
COROT-7c [SEP] constellation | COROT-7c
COROT-7c is an extrasolar planet which orbits the G-type main sequence star COROT-7, located approximately 489 light years away in the constellation Monoceros. It's either a super-Earth or a Neptune-like planet, orbiting at 0.046 AU from the star, taking 3.7 days or 89 hours to make one round trip around the s... | Like COROT-7b, the mass of COROT-7c is weakly constrained, since the radial velocity data is noisy due to the presence of stellar activity. Published mass measurements range from 8.4 Earth masses to 13.5 Earth masses, passing through 12.4 Earth masses and 13.1 Earth masses. This mass range encompasses the Super-Earths ... | 10,970 | zeroshot-train |
EW Aquarii [SEP] constellation | EW Aquarii
EW Aquarii is a star in the constellation Aquarius. A low amplitude Delta Scuti variable, it varies between magnitudes 6.41 and 6.48 over 2.16 hours. Located around 439 light-years distant, it shines with a luminosity approximately 31 times that of the Sun and has a surface temperature of 7163 K. | 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... | 10,971 | zeroshot-train |
Epsilon Capricorni [SEP] constellation | Epsilon Capricorni
Epsilon Capricorni, Latinized from ε Capricorni, is a quadruple star system in the constellation Capricornus. It has the traditional star name Castra or Kastra, meaning "fort" or "military camp" in Latin. Based upon an annual parallax shift of 3.09 mas as seen from the Earth, the star is located abou... | 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.... | 10,972 | zeroshot-train |
G Centauri [SEP] constellation | G Centauri
G Centauri (G Cen) is a star in the constellation Centaurus. It is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.82 and is approximately 450 light years from Earth. | other into egg-shapes.
Tycho Brahe's supernova was visible within Cassiopeia, and the star Tycho G is suspected of being the donor of the material that triggered that explosion.
Features Stars Pattern from Alpha Centauri.
If the Earth's Sun could be observed from α Centauri, the closest star to the Solar System, it wou... | 10,973 | zeroshot-train |
GD 40 [SEP] constellation | GD 40
GD 40 is a white dwarf in the constellation Cetus. The star's spectrum has been found to show traces of external of metal contamination due to disruption of an extrasolar dwarf planet or an asteroid. The disrupted object should have had roughly the same mass of the Solar System asteroid 3 Juno.
See also.
- ZZ Pis... | GD 165
GD 165 is a system of a white dwarf and a brown dwarf of spectral types DA4 + L4, located in constellation Boötes at approximately 103 light-years from Earth.
Nomenclature and observation.
"GD" means "Giclas Dwarf".
The component GD 165 B was discovered in 1988 by Becklin and Zuckerman. It is the first L-type br... | 10,974 | zeroshot-train |
Gliese 1 [SEP] constellation | Gliese 1
Gliese 1 is a red dwarf in the constellation Sculptor, which is found in the southern celestial hemisphere. It is one of the closest stars to the Sun, at a distance of 14.2 light years. Because of its proximity to the Earth it is a frequent object of study and much is known about its physical properties and co... | belt asteroid with a composition similar to that of the largest main belt asteroid, 1 Ceres
- Gliese 176 is a red dwarf star in the constellation of Taurus
- Gliese 176 b is a super-Earth exoplanet in the constellation of Taurus. This planet orbits close to its parent star Gliese 176
In the Bible.
- Minuscule 176 (in t... | 10,975 | zeroshot-train |
Gliese 436 [SEP] constellation | Gliese 436
Gliese 436 is a red dwarf approximately away in the zodiac constellation of Leo. It has an apparent visual magnitude of 10.67, which is much too faint to be seen with the naked eye. However, it can be viewed with even a modest telescope of aperture. In 2004, the existence of an extrasolar planet, Gliese 436b... | Gliese 317 b
Gliese 317 b is an extrasolar planet approximately 50 light-years away in the constellation of Pyxis. The planet was announced in July 2007 to be orbiting the red dwarf star Gliese 317. The planet is a jovian planet that orbits about 95% the distance between Earth to the Sun. Despite of this, it takes abou... | 10,976 | zeroshot-train |
Gliese 674 b [SEP] constellation | Gliese 674 b
Gliese 674 b is an extrasolar planet approximately 15 light years away in the constellation of Ara. This planet orbits tightly around Gliese 674. It is a sub-Neptune-or-Uranus-mass planet either gaseous or rocky. It orbits as close as 0.039 AU from the star and takes only 4.6938 days to orbit. This planet ... | Gliese 317 b
Gliese 317 b is an extrasolar planet approximately 50 light-years away in the constellation of Pyxis. The planet was announced in July 2007 to be orbiting the red dwarf star Gliese 317. The planet is a jovian planet that orbits about 95% the distance between Earth to the Sun. Despite of this, it takes abou... | 10,977 | zeroshot-train |
Groombridge 1618 [SEP] constellation | Groombridge 1618
Groombridge 1618 is a star in the northern constellation Ursa Major. With an apparent visual magnitude of +6.6, it lies at or below the threshold of stars visible to the naked eye for an average observer. It is located close to Earth, at a distance of less than 16 light years. This is a main sequence s... | - "The Black Hole Project" (2013) by C. Sanford Lowe and G. David Nordley. In the novel, Groombridge 34A is one of the stars launching an impactor to make the mini-black hole. It is also the site of an almost terraformed colony planet named New Antarctica.
List of planetary systems in fiction Groombridge 1618.
- "Mindb... | 10,978 | zeroshot-train |
HAT-P-12b [SEP] constellation | HAT-P-12b
HAT-P-12b is an extrasolar planet approximately 468 light years away from Earth, orbiting the 13th magnitude K-type star HAT-P-12, which is located in Canes Venatici constellation. It is a transiting hot Jupiter that was discovered by the HATNet Project on April 29, 2009.
HAT-P-12b is a H/He-dominated gas gia... | 12B (disambiguation)
12B is a 2001 Tamil movie.
12B may also refer to:
- New York State Route 12B, a state highway in the central part of New York
- Missouri Route 12B
- Nebraska Spur 12B
- WASP-12b, an extrasolar planet
- HAT-P-12b, an extrasolar planet
- 12B, a short-lived Mazda Wankel engine
- 12B United States MOS ... | 10,979 | zeroshot-train |
HD 10180 [SEP] constellation | HD 10180
HD 10180 is a Sun-like star in the southern constellation Hydrus that is notable for its large planetary system. Since its discovery, at least seven planets, and possibly as many as nine, have been observed orbiting it, making it potentially the largest of all known planetary systems, including the Solar Syste... | Upsilon Andromedae e
Upsilon Andromedae e is the outermost extrasolar planet orbiting the star Upsilon Andromedae A in the constellation of Andromeda. This planet is one of the most Jupiter-like exoplanets found in terms of mass and semi-major axis.
Discovery.
This planet was discovered on November 22, 2010, but the di... | 10,980 | zeroshot-train |
HD 104304 [SEP] constellation | HD 104304
HD 104304 (24 G. Virginis) is a binary star in the zodiac constellation Virgo. It has an apparent magnitude of 5.54, making it visible to the unaided eye under suitable viewing conditions. The stellar classification of G8 IV means that this is a subgiant star that has left the main sequence and has begun to 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-... | 10,981 | zeroshot-train |
HD 113538 [SEP] constellation | HD 113538
HD 113538 (Gliese 496.1) is a K-type main-sequence star of a late spectral type (K9V) that lies approximately 51 light-years away in the constellation of Centaurus. The star was announced to have a planetary system in 2010.
Planetary system.
Radial velocity variation of HD 113538 was inferred from observation... | responsible. The data is fitted well by a solution including two planets, with an eccentric Saturn-mass planet and a more massive planet on a longer-period orbit—similar to the orbital architecture of the planetary system orbiting HD 163607, though with lower masses. Similar to HD 163607 b, the eccentricity and argumen... | 10,982 | zeroshot-train |
HD 114729 [SEP] constellation | HD 114729
HD 114729 is a 7th magnitude star approximately away in the constellation of Centaurus. Like our Sun (G2V), it is a yellow dwarf (spectral type G0V). It is about the same mass as the Sun, but twice as luminous. That indicates a much greater age, perhaps over 10 billion years. HD 114729 has a co-moving compani... | 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-... | 10,983 | zeroshot-train |
HD 123569 [SEP] constellation | HD 123569
HD 123569 is a star in the constellation Centaurus. Its apparent magnitude is 4.75. | 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-... | 10,984 | zeroshot-train |
HD 128198 [SEP] constellation | HD 128198
HD 128198 is a giant star in the northern constellation of Boötes.
External links.
- HR 5448
- Image HD 128198 | 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-... | 10,985 | zeroshot-train |
HD 129132 [SEP] constellation | HD 129132
HD 129132 is a spectroscopic binary in the constellation Boötes. The stars orbit each other every 9.27 years. | 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-... | 10,986 | zeroshot-train |
HD 13931 b [SEP] constellation | HD 13931 b
HD 13931 b (also known as HIP 10626 b) is an extrasolar planet which orbits the G-type star HD 13931, located approximately 155 light years away in the constellation Andromeda. This planet takes 11.55 years to orbit the star at the average distance of 5.15 AU or 770 Gm. The planet's eccentricity (0.02) is ab... | 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... | 10,987 | zeroshot-train |
HD 154857 c [SEP] constellation | HD 154857 c
HD 154857 c is an extrasolar planet located approximately 224 light-years away in the constellation of Ara, orbiting the star HD 154857. This planet takes about 3470 days (9.5 years) to orbit the star.
The first signs of this planet were noticed on 9 February 2007 by O’Toole in Australia using the method Do... | Mikko Tuomi
Mikko Tuomi is a Finnish astronomer from the University of Hertfordshire, most known for his contributions to the discovery of a number of exoplanets, among them the Proxima Centauri b which orbits the closest star to the Sun. Mikko Tuomi was the first to find indications of the existence of Proxima Centaur... | 10,988 | zeroshot-train |
HD 156668 b [SEP] constellation | HD 156668 b
HD 156668 b is an extrasolar planet orbiting the star HD 156668 78.5 light-years away in the constellation Hercules. It has a minimum mass of 3.1 Earth masses. At the time of discovery it was the second least massive planet discovered by the radial velocity method, subject to the mass/inclination degeneracy... | -34 in the Giclas catalogues. From 1990 to 1993, HD 156668 was observed at least twice and was featured at the 6th annual catalog of the Tokyo Photoelectric Meridian Circle (PMC) where it is one of 6649 stars observed.
Super-Earth.
Andrew Howard announced the discovery of a Super-Earth in orbit around HD 156668. This p... | 10,989 | zeroshot-train |
HD 159868 [SEP] constellation | HD 159868
HD 159868 is a yellow dwarf star approximately 172 light-years away in the constellation of Scorpius. The star is thought to be 3.05 times more luminous than the Sun, yet the metallicity is identical to the Sun.
Planetary system.
- In 2007, a planet of the star was announced by astronomer Simon J. O'Toole. Th... | HD 154857 c
HD 154857 c is an extrasolar planet located approximately 224 light-years away in the constellation of Ara, orbiting the star HD 154857. This planet takes about 3470 days (9.5 years) to orbit the star.
The first signs of this planet were noticed on 9 February 2007 by O’Toole in Australia using the method Do... | 10,990 | zeroshot-train |
HD 1606 [SEP] constellation | HD 1606
HD 1606 is a star in the constellation Andromeda. Although it is suspected of variability, none has been conclusively found, and its apparent magnitude has not been shown to vary from 5.88. Located around away, the star is a blue main-sequence star of spectral type B7V, a massive star that is currently fusing i... | - Berardo Bongiovanni (1560–1563)
- Giovanni Francesco Commendone (September 1563-December 1565)
List To the Polish-Lithuanian Commonwealth.
- Vincenzo Lauro (June 1, 1573 – April 9, 1578)
- Alberto Bolognetti (Alberto Bolognetto) (April 12, 1581-February 1585)
- Claudio Rangoni (bishop of Reggio Emilia) (20 Oct 1598 -... | 10,991 | zeroshot-train |
HD 167042 b [SEP] constellation | HD 167042 b
HD 167042 b is a gas giant extrasolar planet located approximately 163 light-years away in the constellation of Draco, orbiting the star HD 167042. The mass 1.7 M is only minimum since the inclination of the orbital plane is unknown. As it is typical for most known extrasolar planets, it orbits less than 3 ... | It orbits at a distance of 2.7 astronomical units or 400 gigameters and takes 1,208 days or 3.307 years to orbit around Kappa Coronae Borealis.
See also.
- HD 16175 b
- HD 167042 b
- Rho Coronae Borealis b | 10,992 | zeroshot-train |
HD 177809 [SEP] constellation | HD 177809
HD 177809 is a 6th magnitude star in the constellation Lyra, approximately 700 light years away from Earth. It is a red giant star of the spectral type M2III, meaning it possesses a surface temperature of under 3,500 kelvins. In comparison to our Sun, it is much larger and brighter, but its surface is cooler. | 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-... | 10,993 | zeroshot-train |
HD 179949 [SEP] constellation | HD 179949
HD 179949 is a 6th magnitude star in the constellation of Sagittarius. It is a yellow-white dwarf (spectral class F8 V), a type of star hotter and more luminous than our Sun. The star is located about 90 light years from Earth and might be visible under exceptionally good conditions to an experienced observer... | HD 179949 b
HD 179949 b is an extrasolar planet discovered by the Anglo-Australian Planet Search at the Anglo-Australian Observatory, which orbits the star HD 179949. The planet is a so-called "hot Jupiter", a Jupiter-mass planet orbiting very close to its parent star. In this case, orbital distance is almost one-tenth... | 10,994 | zeroshot-train |
HD 181433 [SEP] constellation | HD 181433
HD 181433 is a star located approximately 87 light-years away in the constellation of Pavo (the Peacock). According to SIMBAD, it has a stellar classification of K3III-IV, which puts it on the borderline between being a red giant and a subgiant. This is inconsistent with the fact that its luminosity is only 0... | systems and debris disks.
Six stars with planetary systems have been found. Three planets have been discovered in the system of the orange star HD 181433, an inner super-earth with an orbital period of 9.4 days and two outer gas giants with periods of 2.6 and 6 years respectively. HD 196050 and HD 175167 are yellow G-c... | 10,995 | zeroshot-train |
HD 209458 b [SEP] constellation | HD 209458 b
HD 209458 b, also given the nickname Osiris, is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 159 light-years from the Solar System. The radius of the planet's orbit is 7 million kilometres, about 0.047 astronomical units, or one eighth the radius of Mercury's orbit.... | of core hydrogen fuel and expands into a giant and transfers material to the smaller star.
Twelve star systems have been found to have exoplanets. 51 Pegasi was the first Sun-like star discovered to have an exoplanet companion; 51 Pegasi b (unofficially named Bellerophon) is a hot Jupiter close to its sun, completing a... | 10,996 | zeroshot-train |
HD 212301 [SEP] constellation | HD 212301
HD 212301 is a yellow-white main sequence star located approximately 172 light years (53 parsecs) away in the south circumpolar constellation Octans. The magnitudes are m=7.77 and M=4.16. It has spectral type of F8V. The temperature of the photosphere is 5998 kelvins and have mass 5% more than our Sun. Its ag... | HD 213240 b
HD 213240 b is an extrasolar planet located approximately 133 light-years (41 parsecs) away in the constellation of Grus, orbiting the star HD 213240.
The origin of this known planet came from the country of Switzerland and the astronomer Santos. The date was on April 4, 2001 and the method was Doppler spec... | 10,997 | zeroshot-train |
HD 215497 [SEP] constellation | HD 215497
HD 215497 is a star located approximately 142 light-years away in the constellation of Tucana. It is a K3V star with the characteristics very similar to the Sun. In 2009, two extrasolar planets were discovered orbiting the star.
Planetary system.
Announced in 2009, two extrasolar planets were discovered to be... | light-years away with a super-Earth planet with an orbital period of around 15 days. HD 215497 is an orange star of spectral type K3V around 142 light-years distant. It is orbited by a hot super-Earth every 3 days and a second planet around the size of Saturn with a period of around 567 days. HD 221287 has a spectral t... | 10,998 | zeroshot-train |
HD 220035 [SEP] constellation | HD 220035
HD 220035 is variable star in the equatorial constellation of Aquarius.
External links.
- Image HD 220035 | 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-... | 10,999 | zeroshot-train |
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