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HD 44594 [SEP] constellation | HD 44594
HD 44594 is a star in the southern constellation Puppis. It has an apparent visual magnitude of 6.64, so it can be seen with the naked eye from the southern hemisphere under good viewing conditions. Based upon parallax measurements, it is located at a distance of about from the Earth, giving it an absolute mag... | Â, the energy emission of this star is very similar to the Sun, and thus it is considered a solar analog. The luminosity class 'V' means this is a main sequence star that is generating energy through the thermonuclear fusion of hydrogen at its core. The effective temperature of the outer envelope of HD 44594 is 5,840 K... | 11,100 | zeroshot-train |
HD 53705/53706/53680 [SEP] constellation | HD 53705/53706/53680
HD 53705/53706/53680 is a star system that lies approximately 54 light-years away in the constellation of Puppis. The system consists of four stars in two binaries, making it one of the nearest quadruple star systems.
Component discovery.
HD 53705 was discovered to be a visual binary very early on,... | do not span the full orbit of the companion, but the fit does adjust HD 53680's proper motion to be consistent with the proper motion of HD 53705/53706.
The low inclination of HD 53680 B's orbit reduces the amplitude of the radial velocity variation that it caused on HD 53680 A. In this case, the effect reduced the min... | 11,101 | zeroshot-train |
HD 65216 b [SEP] constellation | HD 65216 b
HD 65216 b is an extrasolar planet located approximately 116 light-years away in the constellation of Carina, orbiting the star HD 65216. This planet was discovered by the Geneva Extrasolar Planet Search Team in 2003. Like most planet candidates so far, it was detected with the radial velocity method.
The pl... | HD 216770
HD 216770 is an 8th magnitude star located approximately 124 light-years away in the constellation of Piscis Austrinus. It is an orange dwarf (spectral type K1 V), and is somewhat dimmer and cooler than our Sun.
In 2003 a planet was announced orbiting it by the Geneva Extrasolar Planet Search Team.
See also.
... | 11,102 | zeroshot-train |
HD 66428 [SEP] constellation | HD 66428
HD 66428 is a G-type main sequence star located approximately 179 light-years away in the constellation of Monoceros. This star is similar to our Sun with an apparent magnitude of 8.25, an effective temperature of 5705 ± 27 K and a solar luminosity 1.28.
Its absolute magnitude is 11.1 while its U-V color index... | 1.14552 solar masses. This precision comes from the Corot mission that measured asteroseismology.
Planetary system.
In July 2006, the discovery of the extrasolar planet HD 66428 b was published in the Astrophysical Journal. It was found from observations at the W. M. Keck Observatory using the radial velocity method. I... | 11,103 | zeroshot-train |
HD 70555 [SEP] constellation | HD 70555
HD 70555 (w Puppis) is a class K2.5II-III (orange giant) star in the constellation Puppis. Its apparent magnitude is 4.83 and it is approximately 1,010 light years away based on parallax. | 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-... | 11,104 | zeroshot-train |
HD 77370 [SEP] constellation | HD 77370
HD 77370, also called b² Carinae (b² Car), is a star in the constellation Carina.
b² Carinae is a yellow-white F-type main sequence dwarf with an apparent magnitude of +5.17. It is approximately 85.4 light years from Earth.
It has a projected rotational velocity of and an effective temperature of 6,609 K. | 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-... | 11,105 | zeroshot-train |
HD 82943 b [SEP] constellation | HD 82943 b
HD 82943 b is an extrasolar planet approximately 89 light-years away in the constellation of Hydra. The planet was announced in 2000 by the Geneva Extrasolar Planet Search Team. The planet is the outermost planet of two.
See also.
- HD 82943 c | HD 168746 b
HD 168746 b is an extrasolar planet orbiting the star HD 168746. It has a minimum mass about one fourth that of Jupiter, so it is most likely a gas giant. It orbits very near the star in a so-called "torch orbit" completing one revolution in only about six and half days.
See also.
- HD 108147 b
- HD 130322 ... | 11,106 | zeroshot-train |
HD 82943 c [SEP] constellation | HD 82943 c
HD 82943 c is an extrasolar planet approximately 89 light-years away in the constellation of Hydra. The planet was announced in 2001 to be orbiting the yellow dwarf star HD 82943. The planet is the innermost planet of two.
See also.
- HD 82943 b | HD 168746 b
HD 168746 b is an extrasolar planet orbiting the star HD 168746. It has a minimum mass about one fourth that of Jupiter, so it is most likely a gas giant. It orbits very near the star in a so-called "torch orbit" completing one revolution in only about six and half days.
See also.
- HD 108147 b
- HD 130322 ... | 11,107 | zeroshot-train |
HD 8535 b [SEP] constellation | HD 8535 b
HD 8535 b (also known as HIP 6511 b) is an extrasolar planet which orbits the G-type main sequence star HD 8535, located approximately 171 light years away in the constellation Phoenix. This planet has at least five-eighths the mass of Jupiter and takes 3.6 years to orbit the star at a semimajor axis of 2.47 ... | 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... | 11,108 | zeroshot-train |
HD 93385 [SEP] constellation | HD 93385
HD 93385 is a star in the southern constellation of Vela. At an apparent visual magnitude of 7.5, it is too faint to be seen with the unaided eye. Parallax measurements made using the Hipparcos satellite show an annual shift of 23.70 milli-arcseconds. This is equivalent to a physical separation of around 138 l... | with a planet 42 times as massive as earth orbiting every 788 days.
HD 93385 is a Sun-like star of spectral type G2/G3V located around 138 light-years away that is orbited by two super-earths with periods of 13 and 46 days and masses 8.3 and 10.1 times that of Earth, respectively.
Features Brown dwarfs.
The discovery o... | 11,109 | zeroshot-train |
HD 96566 [SEP] constellation | HD 96566
HD 96566 (z Carinae, z Car) is a star in the constellation Carina. It is a yellow G-type giant with an apparent magnitude of +4.62 and is approximately 370 light years from Earth.
It has 3.6 times the mass of the Sun. | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,110 | zeroshot-train |
HIP 70849 [SEP] constellation | HIP 70849
HIP 70849 is a 10th magnitude K-type main sequence star located approximately 78 light years away in the constellation Lupus. This star, which resembles a brighter red dwarf, is smaller, cooler, dimmer, and less massive than our Sun. In 2009, a gas giant planet/brown dwarf was found in orbit around it.
There ... | 66, 122, 131, 168, 170, 173, 234, 282.
- Dunne, Aidan. 2008. Rare encounter with sculpture in the spotlight. Irish Times, 6 Feb.
- Kenny, Padraig. 2008. The French Connection. Sunday Tribune, 28 Sep p3.
- Dunne, Aidan, 2005. The Art of Geometry. Irish Times, 23 May, p. 10.
- Woods, Suzanne and Marshall, Catherine. 2005... | 11,111 | zeroshot-train |
HR 7703 [SEP] constellation | HR 7703
HR 7703 (Gliese 783, 279 G. Sagittarii) is a binary star system in the constellation of Sagittarius. The brighter component has an apparent visual magnitude of 5.31, which means it is visible from suburban skies at night. The two stars are separated by an angle of 7.10″, which corresponds to an estimated semima... | 14 stars within 22 light years with a relatively high probability of having habitable planets (a collective probability of 43%). Writing in a "Scientific American" blog in 2011, Caleb Scharf called it "extraordinarily detailed and prescient".
List.
Planets in the Dole List, include.
- Alpha Centari
- Epsilon Eridani
- ... | 11,112 | zeroshot-train |
IC 4756 [SEP] constellation | IC 4756
IC 4756 is an open cluster in the Serpens constellation. It is at a distance of about 1300 light years away from Earth. | SEC, Sep. 2004 – )
- Benjamin S. Santos (IC, August 2004 – October 2005)
"2005–2007":
- Amando M. Tetangco, Jr. (BSP, July 2005 – )
- Fe B. Barin (SEC, Sep. 2004 – )
- Evangeline C. Escobillo (IC, October 2005 – August 2007)
"2007–2010":
- Amando M. Tetangco, Jr. (BSP, July 2005 – )
- Fe B. Barin (SEC, Sep. 2004 -)
- E... | 11,113 | zeroshot-train |
Iota Apodis [SEP] constellation | Iota Apodis
Iota Apodis (ι Aps, ι Apodis) is the Bayer designation for a binary star system in the southern circumpolar constellation of Apus. It is a faint target at an apparent visual magnitude of 5.41, but still visible to the naked eye from suitably dark skies. The distance to this star can be roughly gauged from p... | consisting of ι Apodis, ζ Apodis, β Apodis, γ Apodis, δ Octantis, δ Apodis, η Apodis, α Apodis and ε Apodis. Consequently, ι Apodis itself is known as (, .)
External links.
- Image Iota Apodis | 11,114 | zeroshot-train |
Iota Tauri [SEP] constellation | Iota Tauri
Iota Tauri, Latinized from ι Tauri, is a white-hued star in the zodiac constellation Taurus and an outlying member of the Hyades star cluster. It is visible to the naked eye with an apparent visual magnitude of 4.62, and is located at an estimated distance of about 173 light years based upon parallax measure... | 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... | 11,115 | zeroshot-train |
Kappa Serpentis [SEP] constellation | Kappa Serpentis
Kappa Serpentis, Latinized from κ Serpentis, is a star in the constellation Serpens, in its head (Serpens Caput). It is a red M-type giant with an apparent magnitude of +4.09. It is approximately 382 light years from Earth. It has proper name Gudja since 10 August 2018
Nomenclature.
"κ Serpentis" (Latin... | ", along with Alpha Serpentis, Delta Serpentis, Epsilon Serpentis, Delta Ophiuchi, Zeta Ophiuchi and Gamma Ophiuchi.
In Chinese, (), meaning "Right Wall of Heavenly Market Enclosure", refers to an asterism which represents eleven ancient states in China and which mark the right borderline of the enclosure, consisting o... | 11,116 | zeroshot-train |
Kepler-66 [SEP] constellation | Kepler-66
Kepler-66 is a star with slightly more mass than the Sun in the NGC 6811 open cluster in the Cygnus constellation. It has one confirmed planet, slightly smaller than Neptune, announced in 2013.
External links.
- Kepler-66, The Open Exoplanet Catalogue
- Kepler 66, Exoplanet.eu | 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... | 11,117 | zeroshot-train |
Kepler-70 [SEP] constellation | Kepler-70
Kepler-70, formerly known as KOI-55, is a star in the constellation Cygnus with an apparent visual magnitude of 14.87. This is too faint to be seen with the naked eye; viewing it requires a telescope with an aperture of
A subdwarf B star, Kepler-70 passed through the red giant stage some 18.4 million years ag... | Kepler-9b
Kepler-9b is one of the first planets discovered outside the solar system (exoplanets) by NASA's Kepler Mission. It revolves around the star Kepler-9 within the constellation Lyra. Kepler-9b is the largest of three planets detected in the Kepler system by transit method; its mass is roughly half that of the p... | 11,118 | zeroshot-train |
LSR J1835+3259 [SEP] constellation | LSR J1835+3259
LSR J1835+3259 is a nearby brown dwarf star of spectral class M8.5, located in constellation Lyra, the discovery of which was published in 2003, and it is the 3rd nearest M-type brown dwarf after DEN 1048-3956 and LP 944-020.
Distance.
Trigonometric parallax of this object, measured in 2001–2002 with the... | dwarf star LSR J1835+3259. The mainly red aurora was found to be a million times brighter than the Northern Lights, a result of the charged particles interacting with hydrogen in the atmosphere. It has been speculated that stellar winds may be stripping off material from the surface of the brown dwarf to produce its ow... | 11,119 | zeroshot-train |
MWC 349 [SEP] constellation | MWC 349
MWC 349 is a double (likely, triple) star system in the constellation Cygnus. Its properties are still debated and it may be a massive highly luminous star or a very young less luminous Herbig Ae/Be star. MWC 349 is also a variable star with the designation V1478 Cygni.
MWC 349A and B and a third star.
MWC 349 ... | has not been observed but would help to explain some unusual properties of the system.
Features.
MWC 349B appears to be a relatively conventional hot giant star, but MWC 349A is a very unusual object. It is a supergiant B[e] star, indicating that it is a luminous star with high mass loss and a disc of surrounding mater... | 11,120 | zeroshot-train |
Messier 108 [SEP] constellation | Messier 108
Messier 108 (also known as NGC 3556) is a barred spiral galaxy in the constellation Ursa Major. It was discovered by Pierre Méchain in 1781 or 1782. From the perspective of the Earth, this galaxy is seen almost edge-on.
This galaxy is an isolated member of the Ursa Major Cluster of galaxies in the Virgo sup... | 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... | 11,121 | zeroshot-train |
Messier 50 [SEP] constellation | Messier 50
Messier 50 or M 50, also known as NGC 2323, is an open cluster of stars in the constellation Monoceros. It was recorded by G. D. Cassini before 1711 and independently discovered by Charles Messier on April 5, 1772 while observing Biela's Comet. It is sometimes described as a 'heart-shaped' figure or a blunt ... | 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... | 11,122 | zeroshot-train |
Messier 93 [SEP] constellation | Messier 93
Messier 93 or M93, also known as NGC 2447, is an open cluster in the constellation Puppis. It was discovered by Charles Messier then added to his catalogue of comet-like objects on March 20, 1781. Caroline Herschel, the younger sister of William Herschel, independently discovered M93 in 1783, thinking it had... | 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... | 11,123 | zeroshot-train |
Messier 95 [SEP] constellation | Messier 95
Messier 95, also known as M95 or NGC 3351, is a barred spiral galaxy located about 33 million light-years away in the zodiac constellation Leo. It was discovered by Pierre Méchain in 1781, and catalogued by fellow French astronomer Charles Messier four days later. On 16 March 2012, a supernova was discovered... | M58
M58 or M-58 may refer to:
- Messier 58, a spiral galaxy in the constellation Virgo
- M58 Wolf, an armored vehicle designed to produce a smoke screen
- M58 motorway, a motorway in England
- M58 highway, a federal highway in eastern Siberia, Russian Federation
- M-58 (Michigan highway), a state highway in Michigan
- ... | 11,124 | zeroshot-train |
Messier 98 [SEP] constellation | Messier 98
Messier 98, also known as M98 or NGC 4192, is an intermediate spiral galaxy located about 44.4 million light-years away in the constellation Coma Berenices, about 6° to the east of the bright star Denebola. It was discovered by French astronomer Pierre Méchain on 15 March 1781, along with nearby M99 and M100... | 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... | 11,125 | zeroshot-train |
NGC 1027 [SEP] constellation | NGC 1027
NGC 1027 is an open cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1787. It is visible at the eastern part of the constellation, between two emission nebulae, the Heart and Soul Nebula. However, it is not physically associated with the two nebulae, lying in the foreground, ab... | 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... | 11,126 | zeroshot-train |
NGC 1052 [SEP] constellation | NGC 1052
NGC 1052 is an elliptical galaxy in the constellation Cetus.
Features.
NGC 1052 is located at a distance of around 63 million light years from the Milky Way, and has a LINER-type active galactic nucleus which signals the intense starburst activity in the galaxy's center that were confirmed with observations wi... | NGC 1084
NGC 1084 is an unbarred spiral galaxy in constellation Eridanus. It is at a distance of about 65 million light-years away from Earth. It was discovered by William Herschel on 10 January 1785. The galaxy has multiple spiral arms, which are not well defined. It belongs in the same group with NGC 988, NGC 991, NG... | 11,127 | zeroshot-train |
NGC 1087 [SEP] constellation | NGC 1087
NGC 1087 is an intermediate spiral galaxy in Cetus. The central bar/core is very small with many irregular features in the surrounding disk of material. With the many strange features of NGC 1087, its true nature is still uncertain. It has an extremely small nucleus and a very short stellar bar. Unlike most ba... | for NGC 1087 is 80 million light-years, with a diameter of about 86,800 light-years. The Type II Supernova 1995V is the only recorded supernova in NGC 1087. | 11,128 | zeroshot-train |
NGC 1309 [SEP] constellation | NGC 1309
NGC 1309 is a spiral galaxy located approximately 120 million light-years away, appearing in the constellation Eridanus. It is about 75,000 light-years across, and is about 3/4s the width of the Milky Way. Its shape is classified as SA(s)bc, meaning that it has moderately wound spiral arms and no ring.
Bright ... | 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... | 11,129 | zeroshot-train |
NGC 145 [SEP] constellation | NGC 145
NGC 145, also known as Arp 19, is a barred spiral galaxy in Cetus, notable for its three spiral arms. | NGC 360
NGC 360 is a spiral galaxy located approximately 103 million light-years from the Solar System in the constellation Tucana. It was discovered on 2 November, 1834 by John Herschel. Dreyer, creator of the New General Catalogue described the object as "extremely faint, very much extended 145°, very little brighter... | 11,130 | zeroshot-train |
NGC 1893 [SEP] constellation | NGC 1893
NGC 1893 is an open cluster in the constellation Auriga. It is about 12,400 light years away. The star cluster is embedded in the HII region IC 410.
Images of the star cluster by the Chandra X-ray Observatory suggest that it contains approximately 4600 young stellar objects.
External links.
- Image NGC 1893 | NGC 187
NGC 187 is a barred spiral galaxy located around 3.2 million light-years away in the constellation Cetus, although it can refer to our Milky Way. This galaxy has a stretching bond of clouds in which there's a possibility for stars to be born for as long as that is possible. It was discovered in 1893 by William ... | 11,131 | zeroshot-train |
NGC 2170 [SEP] constellation | NGC 2170
NGC 2170 is a reflection nebula in the constellation Monoceros. It was discovered on October 16, 1784 by William Herschel.
External links.
- The Interactive NGC Catalog Online: NGC 2170
- SIMBAD: NGC 2170
- NASA/IPAC Extragalactic Database: NGC 2170 | NGC 2071
NGC 2071 is a reflection nebula in the constellation Orion. It was discovered on January 1, 1784 by William Herschel. It is part of a group of nebulae, that also includes Messier 78, NGC 2064 and NGC 2067.
External links.
- The Interactive NGC Catalog Online: NGC 2170
- NASA/IPAC Extragalactic Database: NGC 20... | 11,132 | zeroshot-train |
NGC 235 [SEP] constellation | NGC 235
NGC 235 is a lenticular galaxy in the constellation of Cetus. Its companion, PGC 2570, appears in the line of sight of NGC 235, but has no relation with NGC 235. This pair was first discovered by Francis Leavenworth in 1886. Dreyer, the compiler of the catalogue, described the galaxy as "extremely faint, small,... | NGC 1868
NGC 1868 is a globular cluster in the Large Magellanic Cloud in the constellation Dorado. It was discovered by John Herschel in 1834.
External links.
- SIMBAD
- NASA/IPAC
- Flower, P. J., Geisler, D., Olszewski, E. W., & Hodge, P "NGC 1868 - A metal-poor intermediate-age cluster in the Large Magellanic Cloud"... | 11,133 | zeroshot-train |
NGC 26 [SEP] constellation | NGC 26
NGC 26 is a spiral galaxy in the Pegasus constellation. It was discovered on the 14th September 1865 by Heinrich d’Arrest
NGC 26 2MASS (near-infrared) | NGC 4252
NGC 4252 is a spiral galaxy approximately 56 million light-years away from Earth in the constellation of Virgo. It belongs to the Virgo cluster of galaxies.
It was discovered by German astronomer Albert Marth on May 26, 1864.
See also.
- Spiral galaxy
- List of NGC objects (4001–5000)
- Virgo (constellation)
... | 11,134 | zeroshot-train |
NGC 3054 [SEP] constellation | NGC 3054
NGC 3054 is an intermediate spiral galaxy in the constellation Hydra. It was discovered by Christian Heinrich Friedrich Peters in 1859. It is probably in the same galaxy group as NGC 2935.
In January 2006, a supernova (SN 2006T) was observed in NGC 3054.
See also.
- New General Catalogue (NGC)
- NGC 1300
Ext... | 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... | 11,135 | zeroshot-train |
NGC 3669 [SEP] constellation | NGC 3669
NGC 3669 (other designations - UGC 6431, MCG 10-16-135, ZWG 291.67, IRAS11226+5759, PGC 35113) is a barred spiral galaxy in the constellation Ursa Major. It was discovered by William Herschel on March 18, 1790. The galaxy is seen edge-on and appears to be slightly warped. It has a small bulge.
It is a member o... | of the spiral is warped, while its main part features an ordinary differentially rotating disk. The HI gas is also warped and extents more in the western side.
Nearby galaxies.
The galaxy belongs in NGC 3642 group (also known as NGC 3610 group), a galaxy group that also includes NGC 3610, NGC 3619, NGC 3669, NGC 3674 a... | 11,136 | zeroshot-train |
NGC 4088 [SEP] constellation | NGC 4088
NGC 4088 is an intermediate spiral galaxy in the constellation Ursa Major. The galaxy forms a physical pair with NGC 4085, which is located 11′ away.
NGC 4088 is a grand design spiral galaxy. This means that the spiral arms in the galaxy's disk are sharply defined. In visible light, one of the spiral arms appe... | Infrared Spectograph (IRS) on the Spitzer Space Telescope has detected polycyclic aromatic hydrocarbon (PAH) emission.
NGC 3511 forms a pair with NGC 3513, which lies 10.5 arcminutes away from NGC 3511. The two galaxies form a small group, known as the NGC 3511 group, which also includes the galaxy ESO 502-024.
See als... | 11,137 | zeroshot-train |
NGC 4349-127 [SEP] constellation | NGC 4349-127
NGC 4349-127 is a probable red giant approximately 7,097 light-years away in the constellation of Crux. As a member of the open cluster NGC 4349 (hence the name "NGC 4349-127"), it is located about 2000 parsecs (about 6500 light years) from the Sun. Its mass is estimated at 3.9 times Solar, and its age is ... | Lovis and Michel Mayor in June 2007. Lovis had also found three Neptune-mass planets orbiting HD 69830 in May 2006, also in Puppis.
See also.
- NGC 4349-127 b
- PSR B1620-26 b
References.
- SIMBAD NGC 2423 3 b | 11,138 | zeroshot-train |
NGC 51 [SEP] constellation | NGC 51
NGC 51 is a lenticular galaxy in the constellation Andromeda. It has a diameter of 90,000 light-years. The galaxy was discovered on September 7, 1885 by Lewis Swift, who described it as "Pretty faint, pretty small, round, brighter middle."
See also.
- Lenticular galaxy
- List of NGC objects (1–1000)
- Andromeda ... | NGC 7079
NGC 7079 is a barred lenticular galaxy located about 110.58 million light-years away in the constellation of Grus. NGC 7079 is also classified as a LINER galaxy. It is tilted about 51° to the Earth's line of sight. NGC 7079 was discovered by astronomer John Herschel on September 6, 1834.
Physical Characteristi... | 11,139 | zeroshot-train |
NGC 5112 [SEP] constellation | NGC 5112
NGC 5112 is a barred spiral galaxy in the constellation Canes Venatici. This galaxy is in close physical proximity to the edge-on dwarf spiral NGC 5107. | from Space Launch Complex 3E at Vandenberg Air Force Base, and placed OPS 5112 into a transfer orbit. The satellite raised itself into medium Earth orbit using a Star-27 apogee motor.
By 20 June 1978, OPS 5112 was in an orbit with a perigee of , an apogee of , a period of 715.67 minutes, and 63.1 degrees of inclination... | 11,140 | zeroshot-train |
NGC 5490 [SEP] constellation | NGC 5490
NGC 5490 is a radio galaxy in the constellation Boötes.
Gra 1408+17.
Gra 1408+17 is a radio-source in NGC 5490, located at the coordinates: RA , Dec. ; Galactic coordinates J2000 : 009.27 ± 180000, +69.41 ± 180000.
External links.
- Distance
- Image NGC 5490 | 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... | 11,141 | zeroshot-train |
NGC 559 [SEP] constellation | NGC 559
NGC 559, also Caldwell 8, is an open cluster and Caldwell object in the constellation Cassiopeia. It shines at magnitude +9.5. Its celestial coordinates are RA , dec . It is located near the open cluster NGC 637, and the bright magnitude +2.2 irregular variable star Gamma Cassiopeiae. The cluster is 7 arcmins a... | - M107 NGC 6171
- M108 NGC 3556
- M109 NGC 3992
- M110 NGC 205
Herschel 400 objects which are also Caldwell objects.
The Herschel 400 catalogue pre-dates the Caldwell catalogue. The Caldwell catalogue contains 44 objects which are members of the Herschel 400:
- C2 NGC 40 Bow-Tie Nebula
- C6 NGC 6543 Cat's Eye Nebula
- ... | 11,142 | zeroshot-train |
NGC 5750 [SEP] constellation | NGC 5750
NGC 5750 is a barred spiral galaxy with an active galactic nucleus in the constellation Virgo. | Zeta Librae
The Bayer designation ζ Librae, Latinised as zeta Librae (abbreviated ζ Lib / zeta Lib) is shared by several star systems in the constellation Libra. Sources differ about the Flamsteed and Bayer designations that should be applied to four stars:
- HD 137744 (HR 5743), known as ζ and 32 Librae
- HD 137949 (G... | 11,143 | zeroshot-train |
NGC 5792 [SEP] constellation | NGC 5792
NGC 5792 is a barred spiral galaxy about 83 million light-years away in the constellation Libra. There is a magnitude 9.6 star on the northwestern edge of the galaxy. | 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... | 11,144 | zeroshot-train |
NGC 6152 [SEP] constellation | NGC 6152
NGC 6152 is an open cluster of stars located in the constellation Norma. | galactic structure and stellar astrophysics. SALT released its first color images, which marked the achievement of the "first light". This also marked the debut of the fully operating SALTICAM, which is a $600,000 digital camera designed and built for SALT. First light with the full mirror was declared on 1 September 2... | 11,145 | zeroshot-train |
NGC 6520 [SEP] constellation | NGC 6520
NGC 6520 is an open cluster in the constellation Sagittarius. It is magnitude 9.0, diameter 5 arc minutes and class G. It has about 25 stars of magnitude 9 to 12. A dark nebula B86 near its western edge.
References.
- Robert Burnham, Jr, "Burnham's Celestial Handbook: An observer's guide to the universe beyond... | 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... | 11,146 | zeroshot-train |
NGC 6729 [SEP] constellation | NGC 6729
NGC 6729 is a reflection/emission nebula in the constellation Corona Australis. It was discovered by Johann Friedrich Julius Schmidt in 1861.
This fan-shaped nebula opens from the star R Coronae Australis toward the star T CrA to the south-east. R CrA is a pre-main-sequence star in the Corona Australis molecul... | surrounding nebula, NGC 6729, which brightens and darkens with it. The nebula is often compared to a comet for its appearance in a telescope, as its length is five times its width. S Coronae Australis is a G-class dwarf in the same field as R and is a T Tauri star. Nearby, another young variable star, TY Coronae Austra... | 11,147 | zeroshot-train |
NGC 6744 [SEP] constellation | NGC 6744
NGC 6744 is an intermediate spiral galaxy about 30 million light-years away in the constellation Pavo. It is considered as a Milky Way mimic in our immediate vicinity, displaying flocculent (fluffy) arms and an elongated core. It also has at least one distorted companion galaxy (NGC 6744A) superficially simila... | NGC 2336 - another spiral galaxy of similar size and shape
- NGC 1232
External links.
- NGC 6744, a Milky Way-like spiral galaxy
- NGC 6744 (Pav)
- June 4, 2010 – A Sibling of the Milky Way (Wise image of NGC 6744)
- A spiral galaxy that resembles our Milky Way (1 June 2011) | 11,148 | zeroshot-train |
NGC 6850 [SEP] constellation | NGC 6850
NGC 6850 is a spiral galaxy in the constellation Telescopium, discovered by John Herschel in 1836.
External links.
- SIMBAD info page
- VIZIER info page | 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... | 11,149 | zeroshot-train |
NGC 6871 [SEP] constellation | NGC 6871
NGC 6871 is a small, young open cluster in the constellation of Cygnus. The cluster has less than 50 members, most of which are blue and white stars. It is located 5135 light-years from Earth.
External links.
- NGC 6871 at WEBDA
- NGC 6871 at Bernhard Hubl's Astrophotography
- NGC 6871 at Astronomy Magazine | 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... | 11,150 | zeroshot-train |
NGC 6934 [SEP] constellation | NGC 6934
NGC 6934 (also known as Caldwell 47) is a globular cluster in the constellation Delphinus, about 50,000 light years distant. It was discovered by William Herschel on .
External links.
- A Distant Backwater of the Milky Way — ESA/Hubble Picture of the Week | / Clown Face Nebula
- C40 NGC 3626
- C42 NGC 7006
- C43 NGC 7814
- C44 NGC 7479
- C45 NGC 5248
- C47 NGC 6934
- C48 NGC 2775
- C50 NGC 2244
- C52 NGC 4697
- C53 NGC 3115 Spindle Galaxy
- C54 NGC 2506
- C55 NGC 7009 Saturn Nebula
- C56 NGC 246
- C58 NGC 2360
- C59 NGC 3242 Ghost of Jupiter
- C60 NGC 4038 Brighter of two... | 11,151 | zeroshot-train |
NGC 7243 [SEP] constellation | NGC 7243
NGC 7243, also Caldwell 16, is an open cluster and Caldwell object in the constellation Lacerta. It shines at magnitude +6.4. Its celestial coordinates are RA , dec . It is located near the naked-eye stars Alpha Lacertae, 4 Lacertae, an A-class double star, and planetary nebula IC 5217. It lies approximately 2... | – NGC 7243
- VizieR – NGC 7243
- NED – NGC 7243 | 11,152 | zeroshot-train |
OGLE-2005-BLG-071L [SEP] constellation | OGLE-2005-BLG-071L
OGLE-2005-BLG-071L is a distant, magnitude 19.5 galactic bulge star located in the constellation Scorpius, approximately 11000 light years away from the Solar System. The star is probably a red dwarf with a mass 46% of that of our Sun.
Planetary system.
In 2005 an exoplanet was discovered orbiting th... | planets by gravitational microlensing. MicroFUN is based at the Astronomy Department of Ohio State University and coordinates the observation of high-magnification microlensing events. In April 2005, microFUN contributed significantly to the discovery of a Jovian-mass planet (OGLE-2005-BLG-071L), the second planet to b... | 11,153 | zeroshot-train |
OGLE-TR-111 [SEP] constellation | OGLE-TR-111
OGLE-TR-111 is a yellow dwarf star approximately 5,000 light-years away in the constellation of Carina (the Keel). Having an apparent magnitude of about 17, this distant and dim star has not yet been cataloged.
Planetary system.
In 2002 the Optical Gravitational Lensing Experiment (OGLE) survey detected tha... | OGLE-TR-10
OGLE-TR-10 is a distant, magnitude 16 star in the constellation of Sagittarius. It is located near the Galactic Center.
This star is listed as an eclipsing type variable star with the eclipse due to the passage of the planet as noted in the discovery papers.
Planetary system.
This star is home to OGLE-TR-10... | 11,154 | zeroshot-train |
Omicron Ophiuchi [SEP] constellation | Omicron Ophiuchi
Omicron Ophiuchi (ο Oph) is a double star in the constellation Ophiuchus. The apparent magnitudes of its two components are 5.20 and 6.80. | 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... | 11,155 | zeroshot-train |
PSR B1828-11 [SEP] constellation | PSR B1828−11
PSR B1828-11 (also known as PSR B1828-10) is a pulsar approximately 10,000 light-years away in the constellation of Scutum. The star exhibits variations in the timing and shape of its pulses: this was at one stage interpreted as due to a possible planetary system in orbit around the pulsar, though the mode... | PANDA experiment
- PAR thrust
- PEPS effect
- PETRA
- PGM-19 Jupiter
- PHENIX
- PHOBOS experiment
- PHOSFOS
- PICASSO
- PIND
- PITZ
- PLATYPUS
- PLUTO reactor
- PM3 (chemistry)
- POLYGON experiment
- POVM
- PQS (chemical)
- PS210 experiment
- PSR B1828-10
- PSR B1913+16
- PSR J0737-3039
- PSR J1614–2230
- PUREX
- PVLAS... | 11,156 | zeroshot-train |
Phi Herculis [SEP] constellation | Phi Herculis
Phi Herculis (φ Her) is a binary star system in the northern constellation of Hercules. Based upon an annual parallax shift of 15.99 mas as seen from Earth, it is located around 204 light years from the Sun. With a combined apparent visual magnitude of 4.24, it is bright enough to be seen with the naked ey... | the enclosure, consisting of Delta Herculis, Lambda Herculis, Mu Herculis, Omicron Herculis, 112 Herculis, Zeta Aquilae, Theta Serpentis, Eta Serpentis, Nu Ophiuchi, Xi Serpentis and Eta Ophiuchi. Consequently, the Chinese name for Delta Herculis itself is (, ), and represents the state of Wei (魏), together with 33 Cap... | 11,157 | zeroshot-train |
Phi Sagittarii [SEP] constellation | Phi Sagittarii
Phi Sagittarii (Phi Sgr, φ Sagittarii, φ Sgr) is a star in the southern constellation of Sagittarius. With an apparent visual magnitude of 3.17, it is the ninth-brightest star in the constellation and is readily visible to the naked eye. Parallax measurements place it at a distance of roughly from the Ea... | This star, together with Gamma Sagittarii, Delta Sagittarii, Epsilon Sagittarii, Lambda Sagittarii, Sigma Sagittarii, Tau Sagittarii and Phi Sagittarii comprise the "Teapot" asterism.
In Chinese, (), meaning "Dipper", refers to an asterism consisting of Zeta Sagittarii, Phi Sagittarii, Lambda Sagittarii, Mu Sagittarii,... | 11,158 | zeroshot-train |
Pi Virginis [SEP] constellation | Pi Virginis
Pi Virginis (π Vir, π Virginis) is a binary star in the zodiac constellation of Virgo. It is visible to the naked eye with an apparent visual magnitude of 4.64. The distance to this star, based upon parallax measurements, is roughly 380 light years.
This is a spectroscopic binary system with a stellar class... | 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... | 11,159 | zeroshot-train |
Psi Persei [SEP] constellation | Psi Persei
Psi Persei (Psi Per, ψ Persei, ψ Per) is a Be star in the northern constellation of Perseus. It has an apparent visual magnitude of 4.31, so it is visible to the naked eye at night under suitably dark skies. Based on parallax measurements, it is located at a distance of roughly from the Earth.
This star has ... | third house of the White Tiger of the West, representing the boats that Chinese people were reminded to build in case of a catastrophic flood season. Incorporating stars from the northern part of the constellation, it contained Mu, Delta, Psi, Alpha, Gamma and Eta Persei. "Jīshuǐ" (積水), the Swollen Waters, was the four... | 11,160 | zeroshot-train |
R Boötis [SEP] constellation | R Boötis
R Boötis is a Mira variable in the constellation Boötes. It ranges between magnitudes 6.2 and 13.1 over a period of approximately 223 days. | a minimum of 6.79 to a maximum of 7.44 over a period of 5.0 days.
Features Stars Variable stars.
Two of the brighter Mira-type variable stars in the constellation are R and S Boötis. Both are red giants that range greatly in magnitude—from 6.2 to 13.1 over 223.4 days, and 7.8 to 13.8 over a period of 270.7 days respect... | 11,161 | zeroshot-train |
R Virginis [SEP] constellation | R Virginis
R Virginis is a Mira variable in the constellation Virgo. Located approximately distant, it varies between magnitudes 6.1 and 12.1 over a period of approximately 146 days. Its variable nature was discovered by Karl Ludwig Harding in 1809. | 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... | 11,162 | zeroshot-train |
SN 1885A [SEP] constellation | SN 1885A
SN 1885A (also S Andromedae) was a supernova in the Andromeda Galaxy, the only one seen in that galaxy so far by astronomers. It was the first supernova that was ever seen that was outside the Milky Way, though it was not appreciated at the time how far away it was. It is also known as "Supernova 1885".
Discov... | 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 ... | 11,163 | zeroshot-train |
Segue 1 [SEP] constellation | Segue 1
Segue 1 is a dwarf spheroidal galaxy or globular cluster situated in the Leo constellation and discovered in 2006 by Sloan Digital Sky Survey. It is located at a distance of about 23 kpc (about 75,000 light years) from the Sun and moves away from the Sun with the velocity of about 206 km/s. Segue 1 has a notice... | Segue 3
Segue 3 is a faint star cluster of the Milky Way galaxy discovered in 2010 in the data obtained by Sloan Digital Sky Survey. It is located in the Pegasus constellation at the distance of about 17 kpc from the Sun and moves away from it with the velocity of .
Segue 3 is extremely faint—its visible absolute magni... | 11,164 | zeroshot-train |
Sigma Virginis [SEP] constellation | Sigma Virginis
Sigma Virginis (σ Vir, σ Virginis) is a star in the zodiac constellation of Virgo. It can be faintly seen with the naked eye with a baseline apparent visual magnitude of 4.86. Based upon parallax measurements, the distance to this star is roughly 680 light years.
This is an evolved red giant star with a ... | 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... | 11,165 | zeroshot-train |
T Coronae Borealis [SEP] constellation | T Coronae Borealis
T Coronae Borealis ("T CrB"), is a recurring nova in the constellation Corona Borealis. It was first discovered in outburst in 1866 by John Birmingham, although it had been observed earlier as a 10th magnitude star.
Description.
T CrB normally has a magnitude of about 10, which is near the limit of t... | which is a continuation of the Bajcsy-Zsilinszky street leading to Tiszai station. Széchenyi street runs through the Downtown and through most of the city from east to west. The part of the street between the Szinvapark shopping mall and City Hall Square was pedestrianized in the early 1980s, except for the Miskolc tra... | 11,166 | zeroshot-train |
Theta Persei [SEP] constellation | Theta Persei
Theta Persei (Theta Per, θ Persei, θ Per) is a star system 37 light years away from Earth, in the constellation Perseus. It is one of the closest naked-eye stars.
The primary star is a yellowish dwarf (main sequence) star of spectral type F8V, which is somewhat larger and brighter than the Sun, but still w... | , who called it "Divels head" or "Rosch hassatan". A Latin name for Algol from the 16th century was "Caput Larvae" or "the Spectre's Head". Hipparchus and Pliny made this a separate, though connected, constellation.
In Chinese, (), meaning "Mausoleum", refers to an asterism consisting of β Persei, 9 Persei, τ Persei, ι... | 11,167 | zeroshot-train |
V1054 Ophiuchi [SEP] constellation | V1054 Ophiuchi
V1054 Ophiuchi, together with the star Gliese 643, is a nearby quintuple star system, in constellation Ophiuchus at 21.05 light-years. It consists of five stars, all of which are red dwarfs. The alternative designation of Wolf 630 forms the namesake of a moving group of stars that share a similar motion ... | parallax, considering YPC (V1054 Ophiuchi A-Bab and Gliese 643), Hipparcos (Soederhjelm — V1054 Ophiuchi A-Bab and van Leeuwen — Gliese 643) and CTIOPI (V1054 Ophiuchi C) data, is 154.96 ± 0.52 mas, corresponding to a distance 6.453 ± 0.022 pc, or 21.05 ± 0.07 ly.
V1054 Ophiuchi A-Bab (inner triple subsystem).
V1054 Op... | 11,168 | zeroshot-train |
V1094 Scorpii [SEP] constellation | V1094 Scorpii
V1094 Scorpii is a young stellar object in the constellation of Scorpius, located in the young Lupus Star Forming Region.
A planetary system?
Periodic radial velocity variations in the young star V1094 Scorpii had at first been explained by the presence of a substellar object in tight orbit. Currently the... | , Birmingham
- Spire Parkway Hospital (BUPA) – Solihull
- Hospital of St. Cross, Rugby – Warwickshire
- St Michael's Hospital, Warwick – Warwickshire
- Solihull Hospital – Solihull
- County Hospital – Stafford
- Stratford Hospital – Stratford-upon-Avon
- University Hospital Coventry – Coventry
- Walsall Manor Hospital ... | 11,169 | zeroshot-train |
V842 Centauri [SEP] constellation | V842 Centauri
V842 Centauri was a nova which occurred in 1986 in the constellation Centaurus and which reached a brightness of 4.6 mag. It is considered a moderately fast nova, having faded by 3 magnitudes after 48 days. In 2010, it had faded to magnitude 16.5, but was still 2 magnitudes brighter than before the nova e... | rate, gives a similar distance of 1.65 ± 0.54 kpc.
The mass of the white dwarf in V842 Centauri is estimated at 0.88 solar masses. The system is likely seem from a low inclination. An expanding nebula has been detected around V842 Centauri, formed by material ejected during the nova. It has two components, with diamete... | 11,170 | zeroshot-train |
VW Hydri [SEP] constellation | VW Hydri
VW Hydri is a dwarf nova of the SU Ursae Majoris type in the deep southern constellation Hydrus; a star system that consists of a white dwarf and another generally cool star. It is one of the brightest dwarf novae systems in the sky. These systems are characterised by frequent eruptions and less frequent super... | their Bayer designations in 1756. Its name means "male water snake", as opposed to Hydra, a much larger constellation that represents a female water snake. It remains below the horizon for most Northern Hemisphere observers.
The brightest star is the 2.8-magnitude Beta Hydri, also the closest reasonably bright star to ... | 11,171 | zeroshot-train |
WASP-2 [SEP] constellation | WASP-2
WASP-2 is a magnitude 12 orange dwarf star located about 500 light-years away in the Delphinus constellation.
Planetary system.
This star has one extrasolar planet WASP-2b, detected by the SuperWASP project in 2006.
Binary star.
In 2008 a study was undertaken of fourteen stars with exoplanets that were originall... | 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... | 11,172 | zeroshot-train |
WASP-43b [SEP] constellation | WASP-43b
WASP-43b is a transiting planet in orbit around the young, active, and low-mass star WASP-43 in the constellation Sextans. The planet is a Hot Jupiter with a mass twice that of Jupiter, but with a roughly equal radius. WASP-43b was flagged as a candidate by the SuperWASP program before they conducted follow-up... | the closest orbit yet found at the time of WASP-43b's discovery. WASP-43's unusually low mass accounts for WASP-43b's small orbit. Because planets with orbits around stars like WASP-43 are not usually observed, models either suggest that planets like WASP-43b are either uncommon or have short lifetimes caused by a deca... | 11,173 | zeroshot-train |
XX Tauri [SEP] constellation | XX Tauri
XX Tauri (Nova Tauri 1927) was a nova, which appeared in the constellation Taurus in 1927. It is thought to have reached magnitude 6.0. | 90.9 males.
The median income for a household in the village was $48,353, and the median income for a family was $62,186. Males had a median income of $41,024 versus $26,070 for females. The per capita income for the village was $23,539. About 3.4% of families and 4.0% of the population were below the poverty line, inc... | 11,174 | zeroshot-train |
Xi Arietis [SEP] constellation | Xi Arietis
Xi Arietis, Latinized from ξ Arietis, is the Bayer designation for a binary star system in the northern constellation of Aries. It has an apparent visual magnitude of 5.46, and so is dimly visible to the naked eye. Based upon an annual parallax shift of as seen from Earth, it is distant from the Sun. At that... | Guideline tensioner
A guideline tensioner is a hydropneumatic device used on an offshore drilling rig that keeps a positive pulling force on the guidelines from the platform to a template on the seabed.
The guidelines act as a guidance for equipment and tools that must be lowered to the template. If there was no tensio... | 11,175 | zeroshot-train |
Xi Scorpii [SEP] constellation | Xi Scorpii
Xi Scorpii (ξ Sco) is a quintuple star system in the constellation Scorpius. It was assigned this designation by Bayer, although Ptolemy had catalogued the star in Libra. Flamsteed assigned it the designation 51 Librae, but this has fallen out of use since modern constellation boundaries assign the star to S... | and a new engine and generators installed in 2000. In 2010 the Luciole was 'stretched' in a Paris boatyard, when the barge was sliced in two and a new 17 ft section was welded into the bow, providing greater comfort throughout. However, on the front bow deck the curved cargo hatch cover was retained, a reminder of her ... | 11,176 | zeroshot-train |
Xi Serpentis [SEP] constellation | Xi Serpentis
Xi Serpentis, Latinized from ξ Serpentis, is a triple star system in the Serpens Cauda (tail) section of the equatorial constellation Serpens. Based upon an annual parallax shift of 30.98 mas as seen from Earth, it is located 105.3 light years from the Sun. The star system is visible to the naked eye with ... | numerous national and foreign technological and information technology companies. The tech parks are located in Evacuee Trust Complex and Awami Markaz. Awami Markaz houses 36 IT companies while Evacuee Trust house 29 companies.
The economy of Rawalpindi and the surrounding district has a diverse industrial base, but re... | 11,177 | zeroshot-train |
16 Cygni Bb [SEP] constellation | 16 Cygni Bb
16 Cygni Bb or HD 186427 b is an extrasolar planet approximately 69 light-years away in the constellation of Cygnus. The planet was discovered orbiting the Sun-like star 16 Cygni B, one of two solar-mass () components of the triple star system 16 Cygni. It makes one revolution every 799 days and was the fir... | same primordial composition, observations show a small difference in the metallicity of the two 16 Cygni stars. The primary star has an iron abundance of 1.26 times the solar value, compared to 1.13 for the secondary star. A similar trend has been found for all other metals, with the primary component having an average... | 11,178 | zeroshot-train |
21 Arietis [SEP] constellation | 21 Arietis
21 Arietis (abbreviated 21 Ari) is a binary star system in the northern constellation of Aries. "21 Arietis" is the Flamsteed designation. It has a combined apparent visual magnitude is 5.57; the brighter member is magnitude 6.40 while the fainter star is magnitude 6.48. The distance to this star system, bas... | Théophile Gautier first published in 1856
Music.
- Avatar (Swedish band), a Swedish melodic death metal band
- "Avatar" (Avatar album), the third album released by Swedish metal band Avatar
- "Avatar" (Angels and Agony album)
- "Avatar" (Comets on Fire album)
- Avatar Records, a record label
- Savatage or Avatar, an Am... | 11,179 | zeroshot-train |
4 Aquarii [SEP] constellation | 4 Aquarii
4 Aquarii (abbreviated 4 Aqr) is a binary star system in the constellation Aquarius, located approximately 198 light years away from the Sun. "4 Aquarii" is the Flamsteed designation. It is visible to the naked eye as a dim, yellow-white hued star with a combined apparent visual magnitude of 5.99. The system ... | 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... | 11,180 | zeroshot-train |
41 Arietis [SEP] constellation | 41 Arietis
41 Arietis (abbreviated 41 Ari) is a triple star system in the northern constellation of Aries. With an apparent visual magnitude of 3.63, this system is readily visible to the naked eye. It has an annual parallax shift of 19.69 mas, which indicates it is at a distance of from the Sun.
The system consists of... | are not physically related.) The components of A are themselves designated 41 Arietis Aa (formally named Bharani ) and Ab.
Nomenclature.
"41 Arietis" is the system's Flamsteed designation. It does not possess a Greek-letter Bayer designation, since this system was once part of the now-obsolete constellation Musca Borea... | 11,181 | zeroshot-train |
42 Cancri [SEP] constellation | 42 Cancri
42 Cancri (42 Cnc or HD 73785) is a star in the constellation Cancer. Its apparent magnitude is 6.83.
42 Cancri is a member of the Beehive Cluster (NGC 2632). | Lostock College
Lostock College is a mixed, 11-16 secondary modern school in Stretford, Greater Manchester, England. The school enrolls 350 students.
Facilities.
The school previously has specialist status as an Arts College, and funds were used for a new Music Suite with ICT support and a digital recording suite. A su... | 11,182 | zeroshot-train |
55 Ursae Majoris [SEP] constellation | 55 Ursae Majoris
55 Ursae Majoris (55 UMa) is a triple star system in the constellation Ursa Major. Its apparent magnitude is 4.80. Two stars form a close spectroscopic binary with an orbital period of 2.55 days. The third star orbits the central pair every 1873 days. All three stars are A-type main-sequence stars. | a period of uncertainty, and seemed to ensure a pretext for Carol's authoritarianism. By then, Filipescu and Maniu were mainly visible as the sworn enemies of the king, whom they had come to see as an autocratic figure, forcing them into talks about forming the democratic opposition. As early as 1933, rumor spread that... | 11,183 | zeroshot-train |
56 Ursae Majoris [SEP] constellation | 56 Ursae Majoris
56 Ursae Majoris (56 UMa) is a star in the constellation Ursa Major. Its apparent magnitude is 5.03. It is a single-lined spectroscopic binary with an orbital period of about 45 years. | very much in line with his pre-Infinite Crisis appearances. He is shown to be a mechanic/vigilante and a friend to Cave Carson.
In other media.
In other media Television.
- Wild Dog is a recurring character in the live-action series "Arrow", portrayed by Rick Gonzalez. Introduced in season five, Wild Dog is the alias o... | 11,184 | zeroshot-train |
7 Aquarii [SEP] constellation | 7 Aquarii
7 Aquarii, abbreviated 7 Aqr, is a binary star system in the zodiac constellation of Aquarius. "7 Aquarii" is the Flamsteed designation. It is visible to the naked eye with an apparent visual magnitude of 5.5; the brighter component is baseline magnitude 5.62 while the faint secondary is magnitude 11.4. As of... | 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... | 11,185 | zeroshot-train |
Abell 1689 [SEP] constellation | Abell 1689
Abell 1689 is a galaxy cluster in the constellation Virgo nearly 2.2 billion light-years away.
Details.
Abell 1689 is one of the biggest and most massive galaxy clusters known and acts as a gravitational lens, distorting the images of galaxies that lie behind it. It has the largest system of gravitational ar... | of this cluster makes it useful for the study of dark matter and gravitational lensing.
At the time of its discovery in 2008, one of the lensed galaxies, A1689-zD1, was the most distant galaxy found.
See also.
- Abell catalogue
- Gravitational lensing
- List of Abell clusters
External links.
- Galaxy cluster Abell 1689... | 11,186 | zeroshot-train |
Abell 665 [SEP] constellation | Abell 665
Abell 665 is a galaxy cluster in the Abell catalogue in the constellation Ursa Major. It is also known as the only cluster in his 1989 catalog to receive Abell's highest richness class of 5. This means that it contains "at least" 300 galaxies in the magnitude range of m to m+2, where m is the magnitude of the... | , made it an excellent candidate along with 37 other clusters to help determine the Hubble constant using the Sunyaev–Zel'dovich effect in 2006.
Member velocity, cluster velocity dispersion, and X-ray data suggest that Abell 665 is composed of two similar-mass clusters which are at or very close to core crossing, give ... | 11,187 | zeroshot-train |
BG Crucis [SEP] constellation | BG Crucis
BG Crucis is a star in the southern constellation of Crux. A classical Cepheid variable, its apparent magnitude ranges from 5.34 to 5.58 over 3.3428 days. A yellow-white supergiant that pulsates between spectral types F5Ib and G0p, it is around 4.3 times as massive and 2,000 times as luminous as the Sun. | Dean Jagger
Dean Jeffries Jagger (November 7, 1903 – February 5, 1991) was an American film, stage and television actor who won the Academy Award for Best Supporting Actor for his role in Henry King's "Twelve O'Clock High" (1949).
Early life.
Born Dean Ida Jagger, in Columbus Grove or Lima, Ohio, he grew up on a farm. ... | 11,188 | zeroshot-train |
Beta Scorpii [SEP] constellation | Beta Scorpii
Beta Scorpii (β Scorpii, abbreviated Beta Sco, β Sco) is a multiple star system in the southern zodiac constellation of Scorpius. It bore the traditional proper name of Acrab , though the International Astronomical Union now regards that name as applying only to the β Scorpii Aa component.
Components.
Obse... | "B", "C", "E", "Ea" and "Eb" - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).
Beta Scorpii bore the traditional names "Acrab", "Akrab" or "Elacrab", all deriving from the Arabic name () "al-'Aqrab" 'the S... | 11,189 | zeroshot-train |
CFBDSIR 1458+10 [SEP] constellation | CFBDSIR 1458+10
CFBDSIR J145829+101343 (designation abbreviated to CFBDSIR 1458+10, or CFBDSIR J1458+1013) is a binary system of two brown dwarfs of spectral classes T9 + Y0 orbiting each other, located in constellation Boötes about 104 light-years away from Earth.
The smaller companion, CFBDSIR 1458+10B, has a surface... | presented in this paper, and binarity of the other one, CFBDSIR 1458+10, was known before.
Distance.
Trigonometric parallax of CFBDSIR 1458+10, measured under The Hawaii Infrared Parallax Program by Dupuy & Liu in 2012, is 31.3 ± 2.5 mas, corresponding to a distance 31.9 pc, or 104.2 ly.
CFBDSIR 1458+10 distance estima... | 11,190 | zeroshot-train |
COROT-7 [SEP] constellation | COROT-7
COROT-7 (TYC 4799-1733-1) is a G-type main sequence star, slightly smaller and cooler than the Sun. It has an apparent magnitude 11.67, fainter than Proxima Centauri (mag. 11.05), the nearest star to the Sun. This star is located in the Monoceros constellation.
Location and properties.
The star is located in th... | 61 Virginis
61 Virginis (abbreviated 61 Vir) is the Flamsteed designation of a G-type main-sequence star (G7V) slightly less massive than the Sun (which is G2V), located about 27.9 light-years away in the constellation of Virgo. The composition of this star is nearly identical to the Sun.
61 Virginis (G7V) is the first... | 11,191 | zeroshot-train |
Cartwheel Galaxy [SEP] constellation | Cartwheel Galaxy
The Cartwheel Galaxy (also known as ESO 350-40 or PGC 2248) is a lenticular galaxy and ring galaxy about 500 million light-years away in the constellation Sculptor. It is an estimated 150,000 light-years diameter, and has a mass of about solar masses; its outer ring has a circular velocity of .
It was ... | with companion stars, and appear as the white dots that lie along the rim of the X-ray image. The Cartwheel contains an exceptionally large number of these black hole binary X-ray sources, because many massive stars formed in the ring.
External links.
- Galaxy Evolution Simulation:The Cartwheel Galaxy
- Cartwheel Galax... | 11,192 | zeroshot-train |
Cassiopeia Dwarf [SEP] constellation | Cassiopeia Dwarf
The Cassiopeia Dwarf (also known as Andromeda VII) is a dwarf spheroidal galaxy about 2.58 Mly away in the constellation Cassiopeia. The Cassiopeia Dwarf is part of the Local Group and a satellite galaxy of the Andromeda Galaxy (M31).
The Cassiopeia Dwarf was found in 1998, together with the Pegasus Dw... | YZ
YZ, Y.Z., or Yz may refer to:
Astronomy.
- YZ Canis Minoris, a red dwarf star in the constellation Canis Minor
- YZ Cassiopeiae, a star system in the constellation Cassiopeia
- YZ Ceti, a red dwarf star in the constellation Cetus
Other uses.
- Thunderbolt (DC Comics), a fictional character in DC Comics
- "YZ" (film)... | 11,193 | zeroshot-train |
D Centauri [SEP] constellation | D Centauri
D Centauri (D Cen) is a double star in the constellation Centaurus. The system has a combined apparent magnitude of +5.31 and is approximately 570 light years from Earth.
The system is classified as an orange K-type giant. The brighter component has an apparent magnitude of +5.31, while the apparent magnitud... | Cru") and Beta Crucis ("β Cru"), the two brightest stars in the constellation Crux, the Southern Cross, Epsilon Carinae ("ε Car") in Carina, Lambda Scorpii ("λ Sco") in Scorpius and Sigma Sagittarii ("σ Sgr") in Sagittarius. After all twenty-four Greek letters have been assigned, upper and lower case Latin letters are ... | 11,194 | zeroshot-train |
Delta Centauri [SEP] constellation | Delta Centauri
Delta Centauri, Latinized from δ Centauri, is a star in the southern constellation of Centaurus. The apparent visual magnitude of this star is +2.57, making it readily visible to the naked eye. Based upon parallax measurements, it is located at a distance of about from the Earth.
Properties.
δ Centauri i... | SOS members planned long-term affiliation with SOS. Nearly every member surveyed had been exposed to AA, the average rate of AA attendance amongst SOS members in the previous month was 4.5 meetings. A 2007 survey of addiction recovery groups found that religiosity correlated negatively with participation in SOS.
See al... | 11,195 | zeroshot-train |
ESO 280-SC06 [SEP] constellation | ESO 280-SC06
ESO 280-SC06 (also known as ESO 280-6) is a globular cluster 69,800 light years from the Sun in the constellation of Ara. The cluster received this designation when it was catalogued by the European Southern Observatory (ESO) in Chile. Imagery and Hertzsprung-Russell diagrams show a sparsely populated glob... | referred to as "metal-rich" (for example, Terzan 7), while type II are "metal-poor" (for example, ESO 280-SC06).
These two populations have been observed in many galaxies, especially massive elliptical galaxies. Both groups are nearly as old as the universe itself and are of similar ages, but differ in their metal abun... | 11,196 | zeroshot-train |
Epsilon Serpentis [SEP] constellation | Epsilon Serpentis
Epsilon Serpentis, Latinized from ε Serpentis, is a single, white-hued star in the constellation Serpens, in its head (Serpens Caput). It is visible to the naked eye with an apparent visual magnitude of +3.69. Based upon an annual parallax shift of 46.30 mas as seen from Earth, it is located 70 light ... | ", along with Alpha Serpentis, Delta Serpentis, Epsilon Serpentis, Delta Ophiuchi, Zeta Ophiuchi and Gamma Ophiuchi.
In Chinese, (), meaning "Right Wall of Heavenly Market Enclosure", refers to an asterism which represents eleven ancient states in China and which mark the right borderline of the enclosure, consisting o... | 11,197 | zeroshot-train |
Epsilon Sextantis [SEP] constellation | Epsilon Sextantis
Epsilon Sextantis (ε Sex, ε Sextantis) is a solitary star in the equatorial constellation Sextans. With an apparent visual magnitude of 5.24, it is faintly visible to the naked eye on a dark night. The distance to this star, based upon an annual parallax shift of 16.86 mas, is about 193 light years.
T... | V1315 Aquilae
V1315 Aquilae is a cataclysmic variable star located in the constellation of Aquila. It is a type of cataclysmic variable known as a nova-like variable (NL), specifically a SW Sextantis star. Nova-like variables such as these SW Sextantis stars are characterized as having non-magnetic white dwarfs and do ... | 11,198 | zeroshot-train |
G 240-72 [SEP] constellation | G 240-72
G 240-72 (or WD 1748+708, or LHS 455, or GJ 1221) is a nearby degenerate star (white dwarf) of spectral class DQP9.0, located in constellation Draco.
Distance.
G 240-72 is the seventh closest white dwarf (after Sirius B, Procyon B, van Maanen's star, Gliese 440, 40 Eridani B and Stein 2051 B). Its trigonometri... | .
- vO'Malley RL, Godoy G, Hecht EM, Stifelman MD, Taneja SS. Bosniak category IIF designation and surgery for complex renal cysts. J Urol. Sep;182(3):1091-5, 2009.
- Benway BM, Bhayani SB, Rogers CG, Dulabon LM, Patel MN, Lipkin M, Wang AJ, Stifelman MD. Robot assisted partial nephrectomy versus laparoscopic partial n... | 11,199 | zeroshot-train |
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