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GD 356 [SEP] constellation | GD 356
GD 356 is a white dwarf in the constellation of Draco showing an unusual emission of circular polarised light. The star is 65 light years from earth. The class of this white dwarf is DA meaning that it has a cool helium rich atmosphere. This star exhibits emission lines showing the Zeeman effect in the hydrogen ... | 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... | 11,200 | zeroshot-train |
Gliese 758 B [SEP] constellation | Gliese 758 B
Gliese 758 B (often shortened to GJ 758 B) is a brown dwarf orbiting the G-type main sequence star Gliese 758, located approximately 50 light years away, in the constellation Lyra.
Gliese 758 B was detected by direct imaging using the HiCIAO instrument of the Subaru Telescope. The parameters have subsequen... | In November 2009, a team using the HiCIAO instrument of the Subaru Telescope imaged a substellar companion orbiting the star. This object, designated Gliese 758 B, was estimated to be of approximately 10-40 Jupiter masses. A second candidate object was also detected, which was given the designation Gliese 758 C. Follow... | 11,201 | zeroshot-train |
HAT-P-9b [SEP] constellation | HAT-P-9b
HAT-P-9b is an exoplanet approximately 1500 light years away in the constellation Auriga. This planet was found by the transit method on June 26, 2008. It has a mass 78% that of Jupiter and a radius 140% that of Jupiter. As with most transiting planets, this planet is a hot Jupiter, meaning this Jupiter-like p... | 9B
9B, 9b or IX-B may refer to :
- Route 9B (WMATA), a bus route operated by the Washington Metropolitan Area Transit Authority
- Stalag IX-B, a World War II German Army POW camp at Wegscheide close to Bad Orb
- 9B, a 1988 TV Series with Canadian actor Zachary Ansley
- 9B, AccesRail IATA airline designator
- HAT-P-9b, ... | 11,202 | zeroshot-train |
HD 103197 [SEP] constellation | HD 103197
HD 103197 is a 9th magnitude K-type main sequence star located approximately 170 light years away in the constellation Centaurus. The star is smaller, cooler, dimmer, and less massive than our Sun. Its metal content is thirteen-eighths as much as the Sun. In 2009, a gas giant planet was found in orbit around ... | HD 103197 b
HD 103197 b (also known as HIP 57931 b) is an extrasolar planet which orbits the K-type main sequence star HD 103197, located approximately 170 light years away. | 11,203 | zeroshot-train |
HD 104985 b [SEP] constellation | HD 104985 b
HD 104985 b, also named Meztli , is an extrasolar planet approximately 97 parsecs (317 lys) from the SunThe 198-day period planet orbits the yellow giant star HD 104985 (Tonatiuh) at a distance of 0.78 AU. With a mass 6/ times Jupiter it is a gas giant.
Following its discovery in 2003 the planet was designa... | Okayama Planet Search Program
The Okayama Planet Search Program (OPSP) was started in 2001 with the goal of spectroscopically searching for planetary systems around stars. It reported on the detection of 3 new extrasolar planets: (18 Delphini b, ksi Aql b, and 41 Lyncis b), around intermediate-mass G and K giants 18 De... | 11,204 | zeroshot-train |
HD 113538 b [SEP] constellation | HD 113538 b
HD 113538 b is an exoplanet approximately 51 light years away from earth in the constellation Centaurus. It orbits its star(HD 113538) once every 263.3 days, placing it in the outer edge of the habitable zone. However it is most likely a gas giant with no solid surface.
References.
- https://archive.is/2013... | 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... | 11,205 | zeroshot-train |
HD 125612 d [SEP] constellation | HD 125612 d
HD 125612 d is an extrasolar planet which orbits the G-type main sequence star HD 125612, located approximately 172 light years away in the constellation Virgo. The discovery of this planet was announced by the HARPS team on October 19, 2009, together with 31 other planets, including HD 125612 c. | HD 170469
HD 170469 is a yellow subgiant star located approximately 212 light-years away in the constellation Ophiuchus. It has apparent magnitude +8.21 and it is 211.91 ly away.
In 2007, a planet was discovered by the N2K Consortium, led by principal investigators Debra Fischer and Gregory P. Laughlin.
See also.
- HD ... | 11,206 | zeroshot-train |
HD 132029 [SEP] constellation | HD 132029
HD 132029 is a star in the northern constellation of Boötes. It forms a double star with a magnitude 10.2 companion at an angular separation of 4.6″ along a position angle of 110° (as of 2010).
External links.
- HR 5569
- CCDM J14560+3218
- Image HD 132029 | 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-... | 11,207 | zeroshot-train |
HD 139357 [SEP] constellation | HD 139357
HD 139357 is a 6th magnitude K-type giant star located approximately 390 light years from Earth, visible in the constellation Draco. Its mass is four thirds that of our Sun but its radius is 11.47 times larger. However, despite being a giant star, it is only 3.07 billion years old, which is younger than our S... | 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-... | 11,208 | zeroshot-train |
HD 149837 [SEP] constellation | HD 149837
HD 149837 is a binary star in the southern constellation of Ara.
External links.
- HR 6177
- CCDM J16408-6027
- Image of HD 149837 | 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-... | 11,209 | zeroshot-train |
HD 150576 [SEP] constellation | HD 150576
HD 150576 is a double star in the southern constellation of Ara. It has a twelfth magnitude companion at an angular separation of 28.3″ along a position angle of 39° (as of 2000).
External links.
- HR 6207
- Image HD 150576 | 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-... | 11,210 | zeroshot-train |
HD 150706 [SEP] constellation | HD 150706
HD 150706 is a 7th magnitude star in the constellation of Ursa Minor. It is a remarkably Sun-like yellow dwarf (spectral type G0V) being only 6% less massive than the Sun.
Distance to the star, 92 light years, is enough that it is not visible to the unaided eye. However, it is an easy target for binoculars. I... | HD 109749
- HD 150706
- List of extrasolar planets | 11,211 | zeroshot-train |
HD 155358 c [SEP] constellation | HD 155358 c
HD 155358 c is an extrasolar planet orbiting the star HD 155358 located 142 light years away in the constellation Hercules. This is a gas giant which orbits at 1.224 AU and takes 530.3 days to orbit HD 155358. This planet orbits in an eccentric orbit. This planet has at least half the mass of Jupiter.
See a... | 155358 b has mass little bit less than Jupiter but more than Saturn. HD 155358 c has mass half that of Jupiter. However, more accurate masses were needed when inclinations will eventually become known. HD 155358 b orbits at 0.628 AU while c orbits at 1.224 AU.
External links.
- The Extrasolar Planet Encyclopedia: HD 15... | 11,212 | zeroshot-train |
HD 163376 [SEP] constellation | HD 163376
HD 163376 is a star in the constellation Scorpius. Its apparent magnitude is 4.90. | 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-... | 11,213 | zeroshot-train |
HD 17156 [SEP] constellation | HD 17156
HD 17156 is a yellow subgiant star approximately 255 light-years away in the constellation of Cassiopeia. The apparent magnitude is 8.17, which means it is not visible to the naked eye but can be seen with good binoculars. A search for a binary companion star using adaptive optics at the MMT Observatory was ne... | HD 170469
HD 170469 is a yellow subgiant star located approximately 212 light-years away in the constellation Ophiuchus. It has apparent magnitude +8.21 and it is 211.91 ly away.
In 2007, a planet was discovered by the N2K Consortium, led by principal investigators Debra Fischer and Gregory P. Laughlin.
See also.
- HD ... | 11,214 | zeroshot-train |
HD 172044 [SEP] constellation | HD 172044
HD 172044 and BD+33°3154B are two components of a binary star system in the constellation Lyra, approximately 520 light years away from Earth. 5th magnitude HD 172044 is a giant or subgiant star with the spectral type B8II-IIIp... The "p..." signifies that the star has a peculiar spectrum and spectral peculia... | 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-... | 11,215 | zeroshot-train |
HD 175541 b [SEP] constellation | HD 175541 b
HD 175541 b is a jovian planet located approximately 410 light-years away in the constellation of Serpens, orbiting the star HD 175541. This planet was discovered in April 2007. Despite the distance of planet to star slightly more than Earth to the Sun, the period is less than 300 days that orbits in an ecc... | HD 192699
HD 192699 is a yellow subgiant star located approximately 214 light-years away in the constellation of Aquila. It has the apparent magnitude of 6.45. Based on its mass of 1.68 solar, it was an A-type star when it was a main-sequence. In April 2007, a planet was announced orbiting the star, together with HD 17... | 11,216 | zeroshot-train |
HD 185269 b [SEP] constellation | HD 185269 b
HD 185269 b is a hot Jupiter extrasolar planet approximately 171 light years away in the constellation of Cygnus. The minimum mass is slightly less than Jupiter and the orbital period is about one week. Most hot Jupiters are thought to have undergone tidal circularization, making the eccentricity of HD 1852... | 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... | 11,217 | zeroshot-train |
HD 190984 [SEP] constellation | HD 190984
HD 190984 is a 9th magnitude F-type main sequence star located approximately 330 light years away in the constellation Pavo. This star is larger, hotter, brighter, and more massive than our Sun. Also its metal content is one-thirds as much as the Sun. In 2009, a gas giant planet was found in orbit around the ... | HD 5388
HD 5388 (78 G. Phoenicis) is a 7th magnitude F-type main sequence star located approximately 175 light years away in the constellation Phoenix. This star is larger, hotter, brighter, and more massive than our Sun. Also its metal content is half as much as the Sun. In 2009, a gas giant planet was found in orbit ... | 11,218 | zeroshot-train |
HD 217107 c [SEP] constellation | HD 217107 c
HD 217107 c is an extrasolar planet approximately 64 light-years away from Earth in the constellation of Pisces (the Fish). The planet was the second planet to be discovered orbiting the star HD 217107. HD 217107 c's existence was hypothesized in 1998 due to the eccentricity of the inner planet's orbit and ... | Discovery Indication of second planet.
While most planets with orbital periods of less than 10 days have almost circular orbits, HD 217107 b has a somewhat eccentric orbit, and its discoverers hypothesized that this could be due to the gravitational influence of a second planet in the system at a distance of several as... | 11,219 | zeroshot-train |
HD 221246 [SEP] constellation | HD 221246
HD 221246 or NGC 7686 1 is a star in open cluster NGC 7686, and it belongs to the northern constellation of Andromeda. With an apparent visual magnitude of 6.17, it can be viewed by the naked eye only under very favourable conditions. It has a spectral classification of K3III, meaning it is an evolved orange ... | 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-... | 11,220 | zeroshot-train |
HD 28254 b [SEP] constellation | HD 28254 b
HD 28254 b (also known as HIP 20606 b) is an extrasolar planet which orbits the G-type main sequence star HD 28254, located approximately 178 light years away in the constellation Dorado. This planet has at least seven-sixths the mass of Jupiter and takes over three years to orbit the star at a semimajor axi... | sequence. It is estimated to have a mass 11% larger than the Sun's, a radius 57% larger, and an age around 7.8 billion years. It has a luminosity of 1.57 times the solar luminosity and an effective temperature of about 5,600 K. HD 28254 has a low activity level and a larger metallicity than the Sun, with 2.3 times the ... | 11,221 | zeroshot-train |
HD 32518 [SEP] constellation | HD 32518
HD 32518 is a 6th magnitude K-type giant star located 399.7 light years away in the constellation of Camelopardalis. It is 1.13 times more massive, 10.22 times larger, and 41.2 times more luminous than the Sun. However, it has a lower amount of metals than our Sun and the age is older. In August 2009, it was f... | is called γ Ursae minoris, but these names are rarely used. "11 Ursae Minoris" is the Flamsteed designation.
11 Ursae minoris has a detected planet discovered in August 2009.
Planetary system.
11 Ursae minoris b was discovered during a radial velocity survey of 62 K type Red giant stars using the 2m Alfred Jensch teles... | 11,222 | zeroshot-train |
HD 33564 b [SEP] constellation | HD 33564 b
HD 33564 b is an extrasolar planet located approximately 68 light-years away in the constellation of Camelopardalis. This planet orbits around F6V star HD 33564. The planet has an eccentric orbit, ranging in distance from 0.737 AU at periastron to 1.497 AU at apastron.
HD 33564 b is a gas giant in a habitabl... | HD 81040 b
HD 81040 b is a massive, gas giant planet that orbits the star HD 81040. The period is just over 1000 days. It has semimajor axis of 1.94 AU. However, the orbit is extremely eccentric, little over 0.5 in value.
See also.
- HD 33564 b | 11,223 | zeroshot-train |
HD 40307 c [SEP] constellation | HD 40307 c
HD 40307 c is an extrasolar planet orbiting the star HD 40307, located 42 light-years away in the direction of the southern constellation Pictor. The planet was discovered by the radial velocity method, using the HARPS apparatus, in June 2008. Of the six proposed planets in the HD 40307 star system, it is th... | 40307 d was discovered through the Doppler spectroscopy method, which functions by measuring the variations in radial velocity in a star produced by the gravitational effect of orbiting exoplanets. The radial velocities were measured by the High Accuracy Radial Velocity Planet Searcher spectrography system (HARPS) at t... | 11,224 | zeroshot-train |
HD 4732 [SEP] constellation | HD 4732
HD 4732 is a red giant star of magnitude 5.9 located in the constellation Cetus. It is 189 light years from the solar system.
HD 4732 is located in the celestial Southern Hemisphere, although it can be observed from most regions of the Earth. Near Antarctica the star is circumpolar, while it is always below the... | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,225 | zeroshot-train |
HD 50554 [SEP] constellation | HD 50554
HD 50554 is a star approximately away in the constellation Gemini.
Star.
HD 50554 is a yellow-white main-sequence star [F8V] that currently fuse hydrogen in its core. Since the star is 7th magnitude, it is not visible to the unaided eye, but with binoculars or a telescope, it should be easy to see this star. T... | HD 50554 b
HD 50554 b is a Jupiter-sized extrasolar planet with minimum mass 4.4 times that of Jupiter. The planet was announced in 2001 by the European Southern Observatory and confirmed in 2002 using observations from the Lick and Keck telescopes.
See also.
- HD 50499 b | 11,226 | zeroshot-train |
HD 59612 [SEP] constellation | HD 59612
HD 59612 is a class A5Ib supergiant star in the constellation Puppis. Its apparent magnitude is 4.86 and it is approximately 3,100 light years away based on parallax.
It has one companion, B, at magnitude 10.7 and separation 3.0". | 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-... | 11,227 | zeroshot-train |
HD 63454 b [SEP] constellation | HD 63454 b
HD 63454 b is an extrasolar planet located approximately 117 light-years away in the constellation of Chamaeleon, orbiting the star HD 63454. It is at least 38% as massive as Jupiter, and orbits very close to its host star, even closer than the famous 51 Pegasi b. Its close orbit means it belongs to a class ... | 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... | 11,228 | zeroshot-train |
HD 72108 [SEP] constellation | HD 72108
HD 72108 (A Vel, A Velorum) is a star system in the constellation Vela. It is approximately 1640 light years from Earth.
The primary component, HD 72108 A, is a blue-white B-type subgiant with an apparent magnitude of +5.33. It is a spectroscopic binary, whose components are separated by 0.176 arcseconds. At a... | A Velorum
The Bayer designations a Velorum and A Velorum are distinct. Due to , both designations link here. For the star
- a Velorum, see HD 75063
- A Velorum, see HD 72108 | 11,229 | zeroshot-train |
HD 89744 [SEP] constellation | HD 89744
HD 89744 is an F-type subgiant star about 126 light years away in the constellation of Ursa Major. This star has 1.45 times the mass of the Sun, with a projected rotational velocity of 8.0 km s. In 2004, stellar companion HD 89744 B (~0.076 solar mass) with a projected separation of 2,456 AU was detected.
Plan... | HD 89744 b
HD 89744 b is an eccentric Jupiter extrasolar planet orbiting the star HD 89744.
In a simulation of a 10 million year span, this planet swept away all test particles "except for a narrow region near the 8:3 resonance". There can be no planets in this star's habitable zone. Observation has ruled out any plane... | 11,230 | zeroshot-train |
HD 99109 b [SEP] constellation | HD 99109 b
HD 99109 b is an extrasolar planet approximately 197 light-years away in the constellation of Leo. The planet was confirmed in 2006 to be orbiting the orange dwarf star HD 99109. The planet is about one half the mass of Jupiter, classifying the planet as a Jovian planet. The orbital eccentricity is about the... | HD 99109 b has an orbit comparable in eccentricity to the planet Mars in the Solar System but has a mass at least half that of Jupiter. Stability analysis reveals that Earth-size planets could have stable orbits in the planet's Trojan points, located 60 degrees ahead and behind the planet's position in its orbit. | 11,231 | zeroshot-train |
HIP 5158 b [SEP] constellation | HIP 5158 b
HIP 5158 b is an extrasolar planet which orbits the K-type main sequence star HIP 5158, located approximately 130 light years away in the constellation Cetus. This planet was detected by HARPS on October 19, 2009, together with 29 other planets. | HIP 116454 b
HIP 116454 b, or K2-2 b, is an exoplanet orbiting the star HIP 116454, from Earth toward the constellation Pisces. It is in diameter and 12 times as massive as Earth. It was discovered by the NASA "Kepler" spacecraft, and is the first exoplanet discovered during "Kepler" K2 mission. The discovery was annou... | 11,232 | zeroshot-train |
HR 8799 c [SEP] constellation | HR 8799 c
HR 8799 c is an extrasolar planet located approximately 129 light-years away in the constellation of Pegasus, orbiting the 6th magnitude Lambda Boötis star HR 8799. This planet has a mass between 5 and 10 Jupiter masses and a radius from 20 to 30% larger than Jupiter's. It orbits at 38 AU from HR 8799 with an... | limits on its brightness at shorter wavelengths is consistent with trends seen for other young, directly imaged planets like those around HR 8799. In particular, the lower limit of its 1.65–3.8 µm color of 3.1 magnitudes excludes background stars and most brown dwarfs.
The host star is a highly probable member of the L... | 11,233 | zeroshot-train |
Helix Nebula [SEP] constellation | Helix Nebula
The Helix Nebula, also known as NGC 7293, is a planetary nebula (PN) located in the constellation Aquarius. Discovered by Karl Ludwig Harding, probably before 1824, this object is one of the closest to the Earth of all the bright planetary nebulae. The distance, measured by the "Gaia" mission, is 655±13 li... | )
- SEDS - The Helix Nebula (NGC 7293)
- NightSkyInfo – The Helix Nebula (NGC 7293)
- Snopes - Helix Eye of God - Urban Legend
- Helix Nebula (NGC 7293) at Constellation Guide | 11,234 | zeroshot-train |
IM Pegasi [SEP] constellation | IM Pegasi
IM Pegasi is a variable binary star system approximately 329 light-years away in the constellation of Pegasus. With an apparent magnitude of 5.7, it is visible to the naked eye. Increased public awareness of it is due to its use as the guide star for the Gravity Probe B general relativity experiment. It was c... | changes, The Rock was subdivided into Classic Vinyl and Classic Rewind while Big Rock was replaced with Hair Nation. BuzzSaw would have essentially been viewed as the other successor to Big Rock; the arena rock that wasn't played on Hair Nation was generally played on BuzzSaw.
On November 12, 2008 Sirius XM Radio has a... | 11,235 | zeroshot-train |
Kepler-23 [SEP] constellation | Kepler-23
Kepler-23 is a star in the northern constellation of Cygnus, the swan, that is orbited by a planet found to be unequivocally within the star's habitable zone. With an apparent visual magnitude of 14.0, this star is too faint to be seen with the naked eye. | 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... | 11,236 | zeroshot-train |
Kepler-33 [SEP] constellation | Kepler-33
Kepler-33 is a star in the constellation of Cygnus with a system of five known planets. Having begun to evolve off from the main sequence, it has roughly 161.5% of the Sun's radius but only 116.4% of the Sun's mass. Given its mass and temperature, it is likely a subgiant star. The star's distance is not known... | K2-33
K2-33 is an extremely young pre-main-sequence star located about away from the Earth in the constellation of Scorpius. It is known to host one planet, a super-Neptune, named K2-33b. It is also notable for its young age.
Nomenclature and history.
K2-33 also has the 2MASS catalogue number J16101473-1919095 and EPIC... | 11,237 | zeroshot-train |
Kepler-46 [SEP] constellation | Kepler-46
Kepler-46, previously designated KOI-872, is a star located in the constellation Lyra. Observed since 2009 by the Kepler space observatory, it has since been found to possess a planetary system consisting of at least two planets and while it has a similar mass to the Sun (90%) it is significantly older at ten... | -sequence star in the constellation Cygnus, as detected by Kepler, while searching for exoplanets. Various hypotheses have been presented, including comets, asteroids, and an alien civilization.
Mission results 2016.
By May 10, 2016, the Kepler mission had verified 1,284 new planets. Based on their size, about 550 coul... | 11,238 | zeroshot-train |
Kleinmann-Low nebula [SEP] constellation | Kleinmann–Low Nebula
The Kleinmann–Low Nebula (also known as the Orion KL Nebula) is an active star forming region in the Milky Way galaxy. It is a cluster of stars within a molecular cloud.
The Kleinmann–Low Nebula is the at the heart of the Orion Nebula, and is the most active star-forming region in it. Because of th... | . The dust surrounding the Kleinmann-Low Nebula calculated to be approximately 70K. The nebula is estimated to be rather cool at less than 600 Kelvin, yet it is viewed at less than 20 microns to be extremely active based on the infrared light it gives off. Inside of the nebula, the brightest object observed is the Beck... | 11,239 | zeroshot-train |
La Superba [SEP] constellation | La Superba
La Superba (Y CVn, Y Canum Venaticorum) is a strikingly red giant star in the constellation Canes Venatici. It is a carbon star and semiregular variable.
Visibility.
La Superba is a semiregular variable star, varying by about a magnitude over a roughly 160-day cycle, but with slower variation over a larger r... | MS La Superba
MS "La Superba" is a cruiseferry owned and operated by the Italian ferry company Grandi Navi Veloci. It was built at Nuovi Cantieri Apuania in Marina di Carrara, Italy. When it entered service, "La Superba" was the largest passenger ferry operating in the Mediterranean, and one of the largest in the world... | 11,240 | zeroshot-train |
Lambda Arietis [SEP] constellation | Lambda Arietis
Lambda Arietis (λ Ari, λ Arietis) is the Bayer designation for a double star in the northern constellation of Aries. Based upon an annual parallax shift of 25.32 arcseconds, this system is approximately distant from Earth. The pair have a combined apparent visual magnitude of 4.79, which is bright enough... | including Epsilon, Lambda, and Pi Arietis. ε Arietis is a binary star with two white components. The primary is of magnitude 5.2 and the secondary is of magnitude 5.5. The system is 290 light-years from Earth. Its overall magnitude is 4.63, and the primary has an absolute magnitude of 1.4. Its spectral class is A2. The... | 11,241 | zeroshot-train |
Maffei 2 [SEP] constellation | Maffei 2
Maffei 2 is an intermediate spiral galaxy about 10 million light-years away in the constellation Cassiopeia. Maffei 2 and Maffei 1 were both discovered by Paolo Maffei in 1968 from their infrared emission. Maffei 2 lies in the Zone of Avoidance and is about 99.5% obscured by the Milky Way's foreground dust clo... | Mar 1668 Died)
- Giuseppe Spinucci (1668–1695)
- Vincenzo Maria de Rossi, O.F.M. Conv. (23 Jul 1696 – 10 Jun 1698 Died)
- Fabrizio Maffei (22 Dec 1698 – Jun 1723 Died)
- Francesco Antonio Bussolini, O.S.B. (27 Sep 1723 – 20 Mar 1746 Died)
- Innocenzo Gorgoni, O.S.B. (2 May 1746 – 13 Feb 1755 Resigned)
- Gennaro Perrell... | 11,242 | zeroshot-train |
Messier 100 [SEP] constellation | Messier 100
Messier 100 (also known as NGC 4321) is an example of a grand design intermediate spiral galaxy located within the southern part of constellation Coma Berenices. It is one of the brightest and largest galaxies in the Virgo Cluster, located approximately 55 million light-years distant from Earth and has a di... | Messier 41
Messier 41 (also known as M41 or NGC 2287) is an open cluster in the constellation Canis Major. It was discovered by Giovanni Batista Hodierna before 1654 and was perhaps known to Aristotle about 325 BC. M41 lies about four degrees almost exactly south of Sirius, and forms a triangle with it and Nu Canis Maj... | 11,243 | zeroshot-train |
Messier 21 [SEP] constellation | Messier 21
Messier 21 or M21, also designated NGC 6531, is an open cluster of stars in the constellation of Sagittarius. It was discovered and catalogued by Charles Messier on June 5, 1764. This cluster is relatively young and tightly packed. A few blue giant stars have been identified in the cluster, but Messier 21 is... | Pinwheel Galaxy
The Pinwheel Galaxy (also known as Messier 101, M101 or NGC 5457) is a face-on spiral galaxy distanced 21 million light-years (six megaparsecs) away from Earth in the constellation Ursa Major. Discovered by Pierre Méchain on March 27, 1781, it was communicated to Charles Messier who verified its positio... | 11,244 | zeroshot-train |
Messier 86 [SEP] constellation | Messier 86
Messier 86 (also known as M86 or NGC 4406) is an elliptical or lenticular galaxy in the constellation Virgo. It was discovered by Charles Messier in 1781. M86 lies in the heart of the Virgo Cluster of galaxies and forms a most conspicuous group with another large galaxy known as Messier 84. It displays the h... | ) within its borders 5° to 12° west of ε Vir (Vindemiatrix), this constellation is especially rich in galaxies.
Some examples are Messier 49 (elliptical), Messier 58 (spiral), Messier 59 (elliptical), Messier 60 (elliptical), Messier 61 (spiral), Messier 84 (lenticular), Messier 86 (lenticular), Messier 87 (elliptical ... | 11,245 | zeroshot-train |
Messier 91 [SEP] constellation | Messier 91
Messier 91 (also known as NGC 4548 or M91) is a barred spiral galaxy located in the Coma Berenices constellation and is part of the Virgo Cluster of galaxies. M91 is about 63 million light-years away from the earth. It was the last of a group of eight nebulae discovered by Charles Messier in 1781.
Originally... | 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... | 11,246 | zeroshot-train |
Mother Camels [SEP] constellation | Mother Camels
The protecting Mother Camels (Arabic العوائذ "alʽawaʼid") is an asterism in the constellation of Draco described by ancient Arabic nomadic tribes. The asterism was interpreted as a ring of mother camels – Beta Draconis (Rastaban), Gamma Draconis (Eltanin), Nu Draconis (Kuma) and Xi Draconis (Grumium) – su... | 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... | 11,247 | zeroshot-train |
Mz 3 [SEP] constellation | Mz 3
Mz 3 (Menzel 3) is a young bipolar planetary nebula (PN) in the constellation Norma that is composed of a bright core and four distinct high-velocity outflows that have been named lobes, columns, rays, and chakram. These nebulosities are described as: two spherical bipolar lobes, two outer large filamentary hour-g... | . PubMed .
2. United States Patent 8,216,228 - Pachon Mateos, et al. July 10, 2012
http://patft.uspto.gov/netacgi/nph-Parser?Sect1=PTO2&Sect2=HITOFF&p=1&u=%2Fnetahtml%2FPTO%2Fsearch-bool.html&r=1&f=G&l=50&co1=AND&d=PTXT&s1=af-nest&s2=cardioneuroablation&OS=af-nest+AND+cardioneuroablation&RS=af-nest+AND+cardioneuroablat... | 11,248 | zeroshot-train |
NGC 113 [SEP] constellation | NGC 113
NGC 113 is a lenticular galaxy located in the constellation Cetus.br
It was discovered by German astronomer, Ernst Wilhelm Leberecht Tempel, on August 27, 1876. The galaxy lies approximately 210 Million light-years from earth, and is about 80,000 light-years in diameter. | NGC 502
NGC 502, also occasionally referred to as PGC 5034 or UGC 922, is a lenticular galaxy in the constellation Pisces. It located approximately 113 million light-years from the Solar System and was discovered on 25 September 1862 by German astronomer Heinrich Louis d'Arrest.
When the Morphological Catalogue of Gala... | 11,249 | zeroshot-train |
NGC 1535 [SEP] constellation | NGC 1535
NGC 1535 is a planetary nebula in the constellation of Eridanus, discovered by William Herschel on February 1, 1785. It is very similar to the Eskimo Nebula in both color and structure but the central star can be quite difficult to observe visually.
It is sometimes referred to as Cleopatra's Eye Nebula. | 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... | 11,250 | zeroshot-train |
NGC 1860 [SEP] constellation | NGC 1860
NGC 1860 is an open cluster in the Large Magellanic Cloud in the constellation Dorado. It was discovered in 1836 by John Herschel with an 18.7-inch reflecting telescope. | NGC 6366
NGC 6366 is a globular cluster located in the constellation Ophiuchus. It is designated as XI in the galaxy morphological classification scheme and was discovered by the German astronomer Friedrich August Theodor Winnecke on 12 April 1860. It is at a distance of 11,700 light years away from earth.
See also.
- ... | 11,251 | zeroshot-train |
NGC 2040 [SEP] constellation | NGC 2040
NGC 2040 is an open star cluster located 160,000 light years away in the constellation of Dorado. It is a young group of stars in one of the largest star formation regions of the Large Magellanic Cloud. | 05h 30m 17s Dec -66° 53.1′) is an open cluster.
- NGC 2027 (RA 05h 35m 00s Dec -66° 55.0′) is an open cluster.
- NGC 2032 (RA 05h 35m 21s Dec -67° 34.1′; also known as "Seagull Nebula") is a nebula complex that contains four NGC designations: NGC 2029, NGC 2032, NGC 2035 and NGC 2040.
- NGC 2074 (RA 05h 39m 03.0s, Dec ... | 11,252 | zeroshot-train |
NGC 247 [SEP] constellation | NGC 247
NGC 247 is an intermediate spiral galaxy (although it is sometimes classified as a dwarf spiral galaxy) about 11.1 Mly away in the constellation Cetus. This distance was confirmed in late February 2011. Previous measurements showed that the galaxy was about 12.2 Mly away, but this was proved to be wrong. NGC 24... | NGC 508
NGC 508, also occasionally referred to as PGC 5099 or UGC 939, is an elliptical galaxy in the constellation Pisces. It located approximately 247 million light-years from the Solar System and was discovered on 12 September 1784 by British astronomer William Herschel.
Observation history.
Herschel discovered NGC ... | 11,253 | zeroshot-train |
NGC 2997 [SEP] constellation | NGC 2997
NGC 2997 is a face-on unbarred spiral galaxy about 25 million light-years away in the constellation Antlia. It is the brightest galaxy of the NGC 2997 group of galaxies.
NGC 2997 is particularly notable for a nucleus surrounded by a chain of hot giant clouds of ionized hydrogen. It is featured on the cover of ... | NGC 2997 Group
The NGC 2997 group is a group of galaxies about 24.8 million light-years from Earth containing NGC 2997 as a member. It is a group in the Local Supercluster along with the Local Group.
References.
G. De Vaucouleurs, 1975. Nearby Groups of Galaxies, ch. 5. the nearer groups within 10 megaparsecs. Publishe... | 11,254 | zeroshot-train |
NGC 3184 [SEP] constellation | NGC 3184
NGC 3184 is a spiral galaxy approximately 40 million light-years away in the constellation Ursa Major. It has two HII regions named NGC 3180 and NGC 3181.
NGC 3184 houses a high abundance of heavy elements and (SN 1999gi) that was a magnitude 14 Type II supernova detected on December 9, 1999. Other supernovae ... | Itagaki detected a magnitude 17 optical transient 33" east and 61" north of the center of NGC 3184 at coordinates 10 18 19.89 +41 26 28.8. This event may be an outbursting Luminous blue variable (LBV) star. Archival Hubble and Spitzer images of NGC 3184 seem to show no progenitor for optical transient SN 2010dn. SN 201... | 11,255 | zeroshot-train |
NGC 3195 [SEP] constellation | NGC 3195
NGC 3195 is a planetary nebula located in the constellation Chamaeleon. It is the most southern of all the bright sizable planetary nebula in the sky, and remains invisible to all northern observers. Discovered by Sir John Herschel in 1835, this 11.6 apparent magnitude planetary nebula is slightly oval in shap... | star is listed as 15.3V or 16.1B magnitude. Distance is estimated at about 1.7 kpc.
External links.
- The Hubble European Space Agency Information Centre: pictures and information on NGC 3195 | 11,256 | zeroshot-train |
NGC 406 [SEP] constellation | NGC 406
NGC 406 is a spiral galaxy quite similar to the well known Whirlpool Galaxy, located some 65 million light-years away, in the southern constellation of Tucana (the Toucan) and discovered in 1834 by John Herschel. It is described in the New General Catalogue as "faint, very large, round, very gradually a little ... | NGC 1191
NGC 1191 is a lenticular galaxy approximately 406 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.
Together with NGC 1189, NGC 1190, NGC 1192 and NGC 1... | 11,257 | zeroshot-train |
NGC 4147 [SEP] constellation | NGC 4147
NGC 4147 is the "New General Catalogue" identifier for a globular cluster of stars in the northern constellation of Coma Berenices. It was discovered by English astronomer William Herschel on March 14, 1784, who described it as "very bright, pretty large, gradually brighter in the middle". With an apparent vis... | the equivalent of about 16,000 suns, one of the lowest luminosities of any globular cluster. It was discovered by William Herschel in 1784. NGC 4147 is a somewhat dimmer globular cluster, with a much-smaller apparent size.
Features Galaxies.
Features Galaxies Coma Supercluster.
The Coma Supercluster, itself part of the... | 11,258 | zeroshot-train |
NGC 4214 [SEP] constellation | NGC 4214
NGC 4214 is a dwarf barred irregular galaxy located around 10 million light-years away in the constellation Canes Venatici.
Characteristics.
NGC 4214 is both larger and brighter than the Small Magellanic Cloud as well as a starburst galaxy, with the largest star-forming regions ("NGC 4214-I" and "NGC 4214-II")... | less than 3 million years), including a number of star clusters and stellar associations.
NGC 4214 also has two older super star clusters, both with an age of 200 million years and respective masses of 2.6*10. y 1.5*10 solar masses.
See also.
- NGC 4236 - a similar irregular galaxy
External links.
- Hubble Heritage sit... | 11,259 | zeroshot-train |
NGC 4314 [SEP] constellation | NGC 4314
NGC 4314 is a barred spiral galaxy approximately 40 million light-years away in the constellation Coma Berenices. Perhaps the most prominent and unusual feature is its "nuclear starbust ring" of bright young stars. These rings are thought to be due in part to Lindblad resonance. It is thought that this explosi... | NGC 4454
NGC 4454 is a barred spiral galaxy located about 123 million light-years away in the constellation of Virgo. NGC 4454 was discovered by astronomer William Herschel on April 17, 1784.
See also.
- List of NGC objects (4001–5000)
- NGC 4314 | 11,260 | zeroshot-train |
NGC 4627 [SEP] constellation | NGC 4627
NGC 4627 is a dwarf elliptical galaxy in the constellation Canes Venatici. | NGC 1531
NGC 1531 is a dwarf galaxy in the constellation Eridanus that is interacting with the larger spiral galaxy NGC 1532.
It was discovered by John Herschel on 19 October 1835. Although technically classified as a peculiar lenticular galaxy, the galaxy's structure is better described as amorphous.
See also.
- NGC 4... | 11,261 | zeroshot-train |
NGC 4725 [SEP] constellation | NGC 4725
NGC 4725 is an intermediate barred spiral galaxy with a prominent ring structure about 40 million light-years away in the constellation Coma Berenices. NGC 4725 is a Seyfert Galaxy, suggesting an active galactic nucleus containing a supermassive black hole.
NGC 4725 is the brightest member of the Coma I Group.... | Athanassoula tried to set strict constraint to the halo mass, but with partial only success. On the other hand, Morganti et al. found the dark matter fraction to be about 0.6 ± 0.1 at 5Re, with particularly high dark matter fraction inside ∼ 3Re.
Nearby galaxies.
NGC 4494 belongs to the NGC 4565 group, named after the ... | 11,262 | zeroshot-train |
NGC 524 [SEP] constellation | NGC 524
NGC 524 is a lenticular galaxy in the constellation Pisces. It is at a distance of about 90 million light-years away from Earth. In the central bulge of the galaxy is visible gas forming a spiral structure. It is the largest galaxy in a small galaxy group, the NGC 524 group, which is associated with NGC 488 and... | 524" (8.7'). Because of his error the derived position was in error and this was copied into the NGC Catalogue.
In 1913 American astronomer Heber Curtis noted there was nothing at that position and suggested MCG +05-05-030 was in fact NGC 739, based on Edward Crossley's photographs taken at Lick Observatory.
See also... | 11,263 | zeroshot-train |
NGC 5985 [SEP] constellation | NGC 5985
NGC 5985 is a spiral galaxy located in the northern constellation Draco. NGC 5985 was discovered by William Herschel in 1788. | stars. In the centre of NGC 5982 lies a supermassive black hole whose mass is estimated to be (10 ) based on the M–sigma relation. The nucleus may display low level activity and has been categorised as a possible LINER.
NGC 5982 belongs to a galaxy group known as the NGC 5982 group. Other members of the group include t... | 11,264 | zeroshot-train |
NGC 6193 [SEP] constellation | NGC 6193
NGC 6193 is open cluster containing 27 stars in the constellation Ara, visible to the unaided eye. NGC 6193 lies at the center of the Ara OB1 association, which extends over a square degree. The cluster is associated with (and provides the energizing radiation for) neighboring regions of the nebulosity NGC 618... | at least 20 other early B stars in the cluster, of 9th and 10th magnitude.
External links.
- Universität Wien: Plot of stars in NGC 6193 (WEBDA)
- Universität Wien: IDs of stars in NGC 6193 (WEBDA)
- Encyclopedia of Science: Entry for NGC 6193
- Aladin: Image of NGC 6193, centered on HD 150136 | 11,265 | zeroshot-train |
NGC 64 [SEP] constellation | NGC 64
NGC 64 is a barred spiral galaxy discovered by Lewis Swift in 1886, and is located in the Cetus constellation. | NGC 4598
NGC 4598 is a barred lenticular galaxy located in the constellation Virgo. NGC 4598 was discovered by astronomer William Herschel on April 15, 1784.
The distance to NGC 4598 has not been accurately determined; measurements vary from 64 to 102 million light-years. According to the NASA/IPAC Extragalactic Databa... | 11,266 | zeroshot-train |
NGC 66 [SEP] constellation | NGC 66
Namjoons tiddies is a barred spiral galaxy discovered by Frank Muller in 1886, and is located in the Cetus constellation.
See also.
- New General Catalogue
- List of NGC objects
- List of galaxies | NGC 751
NGC 751 is an elliptical galaxy approximately 225 million light-years away from Earth in the constellation of Triangulum. It forms a close pair of interacting galaxies together with the nearby NGC 750 galaxy. The pair is listed as Arp 166 in the Atlas of Peculiar Galaxies (in the category Galaxies with diffuse ... | 11,267 | zeroshot-train |
NGC 7129 [SEP] constellation | NGC 7129
NGC 7129 is a reflection nebula located 3,300 light years away in the constellation Cepheus. A young open cluster is responsible for illuminating the surrounding nebula. A recent survey indicates the cluster contains more than 130 stars less than 1 million years old. NGC 7129 is located just half a degree from... | 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... | 11,268 | zeroshot-train |
NGC 7142 [SEP] constellation | NGC 7142
NGC 7142 is an open cluster about 6,200 light-years away in the constellation Cepheus.
Due to the observational difficulties NGC 7142 presents, it has been an infrequent topic of research. Current known studies include only work being done at the University of Kansas.
Description.
NGC 7142 is located near the ... | this cluster has been especially difficult. Based on NGC 7142's Color-magnitude diagram, it is believed that this cluster is close in age to the old open clusters M 67 and NGC 188 (although age determinations for these two clusters varies wildly in the literature). This makes it one of the oldest open clusters currentl... | 11,269 | zeroshot-train |
NGC 7777 [SEP] constellation | NGC 7777
NGC 7777 is a lenticular galaxy in the constellation of Pegasus.
See also.
- Lenticular galaxy
- List of NGC objects (7000–7840) | 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... | 11,270 | zeroshot-train |
NGC 7822 [SEP] constellation | NGC 7822
NGC 7822 is a young star forming complex in the constellation of Cepheus. The complex encompasses the emission region designated Sharpless 171, and the young cluster of stars named Berkeley 59. The complex is believed to be some 800–1000 pc distant, with the younger components aged no more than a few million y... | Nebula is an example of an unusual shape that an elephant trunk can assume. It has a double helix structure instead of the normal straight column. The double helix is caused by the presence of magnetic fields and electric currents lined up along the trunk axis of the trunks. This makes the filaments of the columns wavy... | 11,271 | zeroshot-train |
NGC 800 [SEP] constellation | NGC 800
NGC 800 is a spiral galaxy located in the constellation of Cetus. It was first observed by the American astronomer Lewis Swift in 1885. | NGC 2264
NGC 2264 is the designation number of the New General Catalogue that identifies two astronomical objects as a single object: the Cone Nebula, and the Christmas Tree Cluster. Two other objects are within this designation but not officially included, the Snowflake Cluster, and the Fox Fur Nebula.
All of the obje... | 11,272 | zeroshot-train |
Nu Persei [SEP] constellation | Nu Persei
Nu Persei (ν Per, ν Persei) is a Class F5, fourth-magnitude star in the constellation Perseus. Nu Persei is a highly luminous yellow-white giant located about 555 light-years from Earth.
Several companions beside the primary have been recorded. B, with magnitude 12.1 and separation 31.6", has its own companio... | and it is now so included in the List of IAU-approved Star Names.
In Chinese, (), meaning "Rolled Tongue", refers to an asterism consisting of Omicron Persei, Nu Persei, Epsilon Persei, Xi Persei, Zeta Persei and 40 Persei. Consequently, the Chinese name for Omicron Persei itself is (), "the Fifth Star of Rolled Tongue... | 11,273 | zeroshot-train |
Omicron Scorpii [SEP] constellation | 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... | can belong to only one constellation. Consequently, the redundant second designation in each pair above has dropped out of use.
Bayer assigned two stars duplicate names by mistake: (duplicated as ) and (duplicated as ). He corrected these in a later atlas, and the duplicate names were no longer used.
Other cases of mul... | 11,274 | zeroshot-train |
Pinwheel Galaxy [SEP] constellation | Pinwheel Galaxy
The Pinwheel Galaxy (also known as Messier 101, M101 or NGC 5457) is a face-on spiral galaxy distanced 21 million light-years (six megaparsecs) away from Earth in the constellation Ursa Major. Discovered by Pierre Méchain on March 27, 1781, it was communicated to Charles Messier who verified its positio... | the Andromeda Galaxy due to their interactions, velocities, and proximity to one another in the night sky. It also has an H II nucleus.
Etymology.
The galaxy gets its name from the constellation Triangulum, where it can be spotted.
The Triangulum Galaxy is sometimes informally referred to as the "Pinwheel Galaxy" by so... | 11,275 | zeroshot-train |
Psi Centauri [SEP] constellation | Psi Centauri
Psi Centauri (ψ Cen, ψ Centauri) is a binary star system in the constellation Centaurus. The primary component is a white A-type subgiant with an apparent magnitude of +4.05. It is approximately 259 light years from Earth. The pair are orbiting each other with a period of 38.81 days and an eccentricity of ... | a democratic society that acknowledges and respects human rights.
Work Prison Work.
Since March 2008 ITEI has carried out programmes of therapy and investigation with prisoners held in detention centres in the cities of La Paz and Cochabamba.
ITEI offers psychological and medical assistance to women and children in pri... | 11,276 | zeroshot-train |
Rho Serpentis [SEP] constellation | Rho Serpentis
Rho Serpentis, Latinized from ρ Serpentis, is a star in the constellation Serpens.
Rho Serpentis is an orange K-type giant with an apparent magnitude of +4.78. It is approximately 375 light years from Earth. | "Yorktown"s Coxswain Joseph Quick rescued a shipmate from drowning while the ship was in port at Yokohama, Japan. For his efforts, Quick was awarded a peacetime Medal of Honor.
"Yorktown" departed the Far East in early 1903 and returned to Mare Island on 3 June. Two weeks later, on the 17th, she was decommissioned.
190... | 11,277 | zeroshot-train |
SN 2003gd [SEP] constellation | SN 2003gd
SN 2003gd was a type II-P supernova occurring in the spiral galaxy Messier 74 in the constellation
Pisces. SN 2003gd was discovered on 12 June 2003 by Robert Evans, using a 0.31m reflector,
and its discovery was confirmed on 13 June 2003 by R. H. McNaught using the 1.0m telescope at the
Siding Spring Observa... | Astronomers were able to identify an object in these pre-supernova images that was in the same position as SN 2003gd, and which is believed to be the supernova's progenitor star. This progenitor star was a red supergiant, consistent with the expectations of existing single-star stellar evolution models. It is the first... | 11,278 | zeroshot-train |
T Cephei [SEP] constellation | T Cephei
T Cephei is a Mira variable star in the constellation Cepheus. Located approximately distant, it varies between magnitudes 5.2 and 11.3 over a period of around 388 days.
Stellar Properties.
T Cephei is a red giant of spectral type M6-9e with an effective temperature 2,400 K, a radius of , a mass of , and a lum... | 1978 by tenor Louis Botto, who sang with the group until 1989, and served as Artistic Director until his death from AIDS in 1997.
As a graduate student of musicology, Botto found that much of the medieval and Renaissance music he was studying was not being performed, and, because of this, he formed the group to perform... | 11,279 | zeroshot-train |
Tau Scorpii [SEP] constellation | Tau Scorpii
Tau Scorpii (τ Sco, τ Scorpii), formally known as Paikauhale , is a star in the southern zodiac constellation of Scorpius. The apparent visual magnitude of Tau Scorpii is +2.8, while parallax measurements yield a distance estimate of roughly 470 light-years (150 parsecs) from Earth.
Description.
Compared to... | Tau Scorpii estimates its effective temperature to be 29,850 kelvins with a luminosity of 20,400 Suns, consistent with an isochronal age of 5 million years and an estimated mass of 14.5–14.7 solar masses.
Nomenclature.
"τ Scorpii" (Latinised to "Tau Scorpii") is the star's Bayer designation.
Tau Scorpii and Sigma Scorp... | 11,280 | zeroshot-train |
Theta Cygni [SEP] constellation | Theta Cygni
Theta Cygni (θ Cygni, θ Cyg) is a star in the northern constellation of Cygnus. It has an apparent visual magnitude of 4.5, so it can be seen from the northern hemisphere with the naked eye in sufficiently dark skies. Based upon parallax measurements, it is at a distance of about from the Earth. It is suspe... | a third iteration, where numeric superscripts were added to distinguish those previously unresolved stars. Examples include Theta Sagittarii ("θ Sgr") later distinguished as Theta¹ Sagittarii ("θ¹ Sgr") and Theta² Sagittarii ("θ² Sgr"), each being their own (physical) star system with two and three stars, respectively.... | 11,281 | zeroshot-train |
Theta Geminorum [SEP] constellation | Theta Geminorum
Theta Geminorum (θ Gem, θ Geminorum) is a single star in the northern zodiac constellation of Gemini. It is visual to the naked eye with an apparent visual magnitude of 3.59. Based upon an annual parallax shift of 17.25 mas, it is about 189 light years distant from the Sun.
This is an evolving A-type su... | the name for the whole constellation; the name means "Star-wreath" and refers to one of the wives of the Pleiades, called "Makalii".
The stars of Auriga feature in Inuit constellations. Quturjuuk, meaning "collar-bones", was a constellation that included Capella (Alpha Aurigae), Menkalinan (Beta Aurigae), Pollux (Beta ... | 11,282 | zeroshot-train |
V849 Ophiuchi [SEP] constellation | V849 Ophiuchi
V849 Ophiuchi or Nova Ophiuchi 1919 was a nova that lit up in 1919 in the constellation Ophiuchus and reached a brightness of 7.4 mag.
External links.
- https://web.archive.org/web/20050909054008/http://www.tsm.toyama.toyama.jp/curators/aroom/var/nova/1910.htm | on .
Publications.
- Stubbs collected and edited Steve Biko's writings and published them as "I Write what I Like" | 11,283 | zeroshot-train |
W Ursae Majoris [SEP] constellation | W Ursae Majoris
W Ursae Majoris (W UMa) is the variable star designation for a binary star system in the northern constellation of Ursa Major. It has an apparent visual magnitude of about 7.9, which is too faint to be seen with the naked eye. However, it can be viewed with a small telescope. Parallax measurements place... | The same day, the team signed Timo Pérez to a minor-league contract.
- On February 3, the Tigers avoided arbitration with starting pitcher Justin Verlander by signing him to a one-year, $3.7 million contract.
- On February 4, the organization outrighted pitcher Eddie Bonine to the Mud Hens after clearing waivers. He ha... | 11,284 | zeroshot-train |
WASP-4b [SEP] constellation | WASP-4b
WASP-4b is an extrasolar planet approximately 880 light-years away in the constellation of Phoenix.
The planet was the discovered by the SuperWASP project using cameras in South Africa. After its discovery, the mass of the WASP-4 b was determined by measuring the radial velocity of WASP-4, which confirmed that ... | TrES-4b
TrES-4b is an extrasolar planet, and one of the largest exoplanets ever found, after WASP-12b, WASP-17b, CT Chamaeleontis b (though the latter may be a brown dwarf) and GQ Lupi b. It was discovered in 2006, and announced in 2007, by the Trans-Atlantic Exoplanet Survey, using the transit method. It is approximat... | 11,285 | zeroshot-train |
WOH G64 [SEP] constellation | WOH G64
WOH G64 (IRAS 04553-6825) is a red hypergiant (RHG) or red supergiant (RSG) star in the Large Magellanic Cloud (LMC) satellite galaxy in the southern constellation of Dorado. It is one of the largest known stars, with a radius of , corresponding to a volume some 3.65 to 17 billion times bigger than the Sun. It ... | the LMC. In 2007, observers using the Very Large Telescope (VLT) showed that WOH G64 is surrounded by a torus-shaped cloud. Westerlund also discovered another notable cool hypergiant star, Westerlund 1-26, found in the massive super star cluster Westerlund 1 in the constellation Ara.
WOH G64 was also discovered to be a... | 11,286 | zeroshot-train |
XO-4 [SEP] constellation | XO-4
XO-4 is a star located approximately 896 light-years away from Earth in the Lynx constellation. It has a magnitude of about 11 and cannot be seen with the naked eye but is visible through a small telescope. A search for a binary companion star using adaptive optics at MMT Observatory was negative.
Planetary system... | XO-1
XO-1 is a magnitude 11 G-type main-sequence star star located approximately 536 light-years away in the constellation Corona Borealis. XO-1 has a mass and radius similar to the Sun.
In 2006 the extrasolar planet XO-1b was discovered orbiting XO-1 by the transit method using the XO Telescope.
Planetary system.
The ... | 11,287 | zeroshot-train |
XO-4b [SEP] constellation | XO-4b
XO-4b is an extrasolar planet approximately 956 light years away in the constellation of Lynx. This planet was found by the transit method by McCullough in May 2008. The planet has mass and radius . This planet orbits very close to the F-type parent star, as it is typical for transiting planets, classing this pla... | 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... | 11,288 | zeroshot-train |
Zeta Apodis [SEP] constellation | Zeta Apodis
Zeta Apodis, Latinized from ζ Apodis, is the Bayer designation for a star in the southern constellation of Apus. It has an apparent visual magnitude of +4.78, which is bright enough to allow it to be seen with the naked eye. The distance to this star is known from parallax measurements to be around .
The sp... | spectral type K3III, located 550 ± 10 light-years away, with a magnitude of 5.3. The separate components can be resolved with the naked eye.
The fifth-brightest star is Zeta Apodis at magnitude 4.8, a star that has swollen and cooled to become an orange giant of spectral type K1III, with a surface temperature of 4649 K... | 11,289 | zeroshot-train |
Zeta Cygni [SEP] constellation | Zeta Cygni
Zeta Cygni (ζ Cyg) is a binary star system in the northern constellation of Cygnus, the swan. It has an apparent visual magnitude of 3.26 and, based upon parallax measurements, is about away.
The primary component, ζ Cyg A is a giant star with a spectral type of G8 IIIp. Its most likely status is as a red cl... | T Vulpeculae
T Vulpeculae is a possible binary star system in the northern constellation of Vulpecula, near the star Zeta Cygni, close to the pair 31 Vulpeculae and 32 Vulpeculae. It is visible to the naked eye with an apparent visual magnitude that ranges around 5.75. The distance to this system is around 1,900 light ... | 11,290 | zeroshot-train |
101 Virginis [SEP] constellation | 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... | Virginis
Virginis may refer to :
Astronomy.
- Stars in the constellation Virgo.
- Alpha Virginis is the brightest star in the constellation Virgo.
- 61 Virginis is a star located about 27.8 light-years away in the constellation of Virgo.
- Etc.
- 101 Virginis or CY Boötis is a variable star in the Bootes constellation.... | 11,291 | zeroshot-train |
12 Ophiuchi [SEP] constellation | 12 Ophiuchi
12 Ophiuchi is a variable star in the constellation Ophiuchus. No companions have yet been detected in orbit around this star, and it remains uncertain whether or not it possesses a dust ring.
This star is categorized as a BY Draconis variable, with variable star designation V2133. The variability is attrib... | 2015 – "When Dad Showed Me the Universe"
- 2018 - "My Little Small"
External links.
- Ulf Stark on www.forfatterweb.dk (Danish)
-
- Ulf Stark (written on Danish)
- Ulf Stark on Bonnier Carlsen's website
- Ulf Stark on Gecko Press's website | 11,292 | zeroshot-train |
14 Herculis b [SEP] constellation | 14 Herculis b
14 Herculis b or 14 Her b is an extrasolar planet approximately 58.5 light-years away in the constellation of Hercules. The planet was found orbiting the star 14 Herculis, with a mass that would likely make the planet a Jovian planet roughly the same size as Jupiter but much more massive. It was discovere... | campaigns (1757–1759) and participated in the last battles of the Seven Years' War. At the end of that war, in 1763, his regiment was disbanded and he went into retirement until the French Revolution.
A municipal officer of Béziers in 1790, on 9 September 1791 he was elected to the National Assembly as député for Hérau... | 11,293 | zeroshot-train |
20 Leonis Minoris [SEP] constellation | 20 Leonis Minoris
20 Leonis Minoris is a binary star system in the northern constellation of Leo Minor. It is faintly visible to the naked eye, having an apparent visual magnitude of +5.4. Based upon an annual parallax shift of 66.46 mas, it is located 49 light years from the Sun. The star has a relatively high proper ... | . 46 Leonis Minoris, an orange giant of magnitude 3.8, is located some 95 light-years from Earth. At magnitude 4.4, Beta Leonis Minoris is the second-brightest star and the only one in the constellation with a Bayer designation. It is a binary star, the brighter component of which is an orange giant and the fainter a y... | 11,294 | zeroshot-train |
2MASS 0939-2448 [SEP] constellation | 2MASS 0939−2448
2MASS 0939−2448 (full designation is 2MASS J09393548−2448279) is a probable system of two nearby T-type brown dwarfs, located in constellation Antlia at 17.4 light-years from Earth.
Discovery.
2MASS 0939−2448 was identified as a brown dwarf through analysis of data from the 2MASS survey by Tinney "et al... | final data release for 2MASS occurred in 2003, and is served by the Infrared Science Archive. The goals of this survey included:
- Detection of galaxies in the "Zone of Avoidance", a strip of sky obscured in visible light by our own galaxy, the Milky Way.
- Detection of brown dwarfs. 2MASS discovered a total of 173, in... | 11,295 | zeroshot-train |
35 Arietis [SEP] constellation | 35 Arietis
35 Arietis (abbreviated 35 Ari) is a binary star in the northern constellation of Aries. "35 Arietis" is the Flamsteed designation. It is approximately distant from the Earth, based upon an annual parallax shift of 9.51 mas. This star is visible to the naked eye with an apparent visual magnitude of 4.64.
Thi... | ", and "sickle", which was associated with the ritual sacrifice of cattle. This name was shared by the 16th lunar mansion, the location of the full moon closest to the autumnal equinox. The lunar mansion represented the area where animals were gathered before sacrifice around that time. This constellation has also been... | 11,296 | zeroshot-train |
62 Arietis [SEP] constellation | 62 Arietis
62 Arietis is a single star in the northern constellation of Aries, a few degrees to the north of Tau Arietis. "62 Arietis" is the Flamsteed designation. It is visible to the naked eye as a dim, yellow-hued star with an apparent visual magnitude of 5.52. Based upon an annual parallax shift of , it is approxi... | 's first winter pops series, the "8 O'Clock Pops". When the Cincinnati Symphony Orchestra board of trustees created the Cincinnati Pops Orchestra in 1977, Kunzel was named conductor. The Pops became the larger of Cincinnati's two orchestras, as all of Max Rudolf's symphony orchestra also played for the Pops year-round.... | 11,297 | zeroshot-train |
68 Cancri [SEP] constellation | 68 Cancri
68 Cancri (68 Cnc) is a star in the constellation Cancer. Its apparent magnitude is 7.38. | Trigonopterus fulgidus
Trigonopterus fulgidus is a species of flightless weevil in the genus "Trigonopterus" from Indonesia.
Etymology.
The specific name is derived from the Latin word "fulgidus", meaning "shining" or "gleaming".
Description.
Individuals measure 2.38–3.78 mm in length. The legs, head, and underside are... | 11,298 | zeroshot-train |
85 Pegasi [SEP] constellation | 85 Pegasi
85 Pegasi is a multiple star system 39.5 light years away in the constellation of Pegasus. The primary component is sixth magnitude 85 Pegasi A, which is a yellow dwarf like the Sun. The secondary component, 85 Pegasi B, is a ninth magnitude orange dwarf that takes 26.28 years to orbit at 10.3 AU around the p... | in Yekaterinburg before leaving as a free agent to sign a one-year contract with fellow KHL club, HC Dinamo Minsk, on June 22, 2019. | 11,299 | zeroshot-train |
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