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Zeta Leporis [SEP] constellation | Zeta Leporis
Zeta Leporis, Latinized from ζ Leporis, is a star approximately away in the southern constellation of Lepus. It has an apparent visual magnitude of 3.5, which is bright enough to be seen with the naked eye. In 2001, an asteroid belt was confirmed to orbit the star.
Stellar components.
Zeta Leporis has a st... | Hawaii, was used more accurately to constrain the radius of the dust. It was found to lie within a 5.4 AU radius. The temperature of the dust was estimated as about 340 K. Based on heating from the star, this could place the grains as close as 2.5 AU from Zeta Leporis.
It is now believed that the dust is coming from a ... | 11,400 | zeroshot-train |
Zeta Lupi [SEP] constellation | Zeta Lupi
ζ Lupi (Latinised as Zeta Lupi) is a wide double star in the constellation Lupus, consisting of an orange-hued primary and a fainter secondary with a golden-yellow hue. It is visible to the naked eye with a combined apparent visual magnitude of 3.41. Based upon an annual parallax shift of 27.80 mas as seen fr... | Lobbying in the United States
Lobbying in the United States describes paid activity in which special interests hire well-connected professional advocates, often lawyers, to argue for specific legislation in decision-making bodies such as the United States Congress. It is a highly controversial phenomenon, often seen in... | 11,401 | zeroshot-train |
18 Delphini [SEP] constellation | 18 Delphini
18 Delphini (abbreviated 18 Del), also named Musica , is a yellow giant star approximately 249 light-years from Earth in the constellation of Delphinus of the low northern hemisphere. An object believed to be an extrasolar planet (designated 18 Delphini b or Arion) orbits the star.
Nomenclature.
18 Delphini... | territory from the Diocese of Grand Rapids to form the new Diocese of Kalamazoo.
History Reports of Sex Abuse.
On May 24, 2019, it was revealed that five priests who served in the Diocese of Lansing, as well as the Archdiocese of Detroit and the Diocese of Kalamazoo were charged with sex abuse. Michigan Attorney Genera... | 11,402 | zeroshot-train |
31 Crateris [SEP] constellation | 31 Crateris
31 Crateris is a binary star system in the constellation Corvus. Varying between apparent magnitudes 5.19 and 5.23 over 1.48 days, it has the variable star designation of TY Corvi. It is actually a remote system with a hot blue-white star of spectral type B1.5V and a companion about which little is known. T... | Eta Crateris
Eta Crateris (η Crateris) is a solitary star in the southern constellation of Crater. It marks the lip of the tilted bowl on the left side in the constellation. Eta Crateris lies in the sky NE of Zeta Crateris and NNW of 31 Crateris, the three stars forming an almost perfect right triangle with Eta at the ... | 11,403 | zeroshot-train |
47 Aquarii [SEP] constellation | 47 Aquarii
47 Aquarii, abbreviated 47 Aqr, is a star in the zodiac constellation of Aquarius. "47 Aquarii" is its Flamsteed designation. It is a faint star but visible to the naked eye in good seeing conditions, having an apparent visual magnitude of 5.135. Based upon an annual parallax shift of , it is located 181 lig... | 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... | 11,404 | zeroshot-train |
52 Arietis [SEP] constellation | 52 Arietis
52 Arietis (abbreviated 52 Ari) is a triple star system in the northern constellation of Aries. "52 Arietis" is the Flamsteed designation. The combined apparent magnitude is +5.46, which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 6.05 mas, the system is ro... | , Leno has been the Grand Marshal for the Love Ride, a motorcycle charity event which since its founding in 1984 has raised nearly $14 million for charities benefiting muscular dystrophy research, Autism Speaks, and in 2001, the September 11 attacks recovery.
Personal life Vehicle collection.
Leno owns approximately 28... | 11,405 | zeroshot-train |
61 Virginis d [SEP] constellation | 61 Virginis d
61 Virginis d (abbreviated 61 Vir d) is a proposed exoplanet orbiting the 5th apparent-magnitude G-type main-sequence star 61 Virginis in the constellation Virgo. 61 Virginis d would have a minimum mass of 22.9 times that of Earth and orbits nearly one-half the distance to the star as Earth orbits the Sun... | 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... | 11,406 | zeroshot-train |
65 Aquarii [SEP] constellation | 65 Aquarii
65 Aquarii (abbreviated 65 Aqr) is a star in the constellation of Aquarius. "65 Aquarii" is its Flamsteed designation. Its apparent magnitude is 7.04. | 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... | 11,407 | zeroshot-train |
91 Aquarii b [SEP] constellation | 91 Aquarii b
91 Aquarii b, also known as HD 219449 b, is an extrasolar planet orbiting in the 91 Aquarii system approximately 148 light-years away in the constellation of Aquarius. It orbits at the average distance of 105 Gm from its star, which is slightly closer than Venus is to the sun (108 gm). The planet takes hal... | HD 10647 b
HD 10647 b, also catalogued as q Eridani b, is an extrasolar planet approximately 57 light-years away in the constellation of Eridanus (the River). The planet is a mid-Jovian that orbits 103% farther from the star than Earth to the Sun. It takes about 33 months to orbit with semi-amplitude of 17.9 m/s.
See a... | 11,408 | zeroshot-train |
AFGL 2591 [SEP] constellation | AFGL 2591
AFGL 2591 is a star forming region in the constellation Cygnus. Its dense cloud of gas and dust make its interior invisible to optical telescopes. Images in the infrared show a bright young stellar object, with an associated reflection nebula seen as a glowing cone projecting from the young star. A cluster of... | AFGL 2298
AFGL 2298, also known as IRAS 18576+0341, is a luminous blue variable star (LBV) located in the constellation Aquila, very close to the galactic plane. Its distance is not well known; it may be anywhere between and light years (7,000 to 13,000 parsecs) away from the Earth. Despite being extremely luminous, it... | 11,409 | zeroshot-train |
AW Canum Venaticorum [SEP] constellation | AW Canum Venaticorum
AW Canum Venaticorum is a variable star in the constellation Canes Venatici. It is visible to the naked eye with a nominal apparent visual magnitude of 4.76. The distance to this star, as measured from its annual parallax shift of , is around 620 light years. It is moving closer with a heliocentric... | European manner "and" the Longhouse manner, with the Longhouse ceremony usually held first.
Culture Longhouses.
Replicas of seventeenth-century longhouses have been built at landmarks and tourist villages, such as Kanata Village, Brantford, Ontario, and Akwesasne's "Tsiionhiakwatha" interpretation village. Other Mohawk... | 11,410 | zeroshot-train |
Abell 754 [SEP] constellation | Abell 754
Abell 754 is a galaxy cluster in the constellation Hydra that was formed from the collision of two smaller clusters. This collision, which began about 300 million years ago, is ongoing, and the system is still disturbed. Eventually, the cluster will reach a level of equilibrium in a few billion years.
See als... | the prototype relic source 1253 + 275), Abell 2255 and Abell 2256, which contain both a relic and a halo (as do Abell 225, Abell 521, Abell 754, Abell 1300, Abell 2255 and Abell 2744). The cluster Abell 3667 contains two very luminous, almost symmetric
relics with a separation of more than 5 Mpc, as does ZwCl 2341.1+00... | 11,411 | zeroshot-train |
Beta Sextantis [SEP] constellation | Beta Sextantis
Beta Sextantis, Latinized from β Sextantis, is a variable star in the equatorial constellation of Sextans. With an apparent visual magnitude of 5.07, it is faintly visible to the naked eye on a dark night. According to the Bortle scale, it can be viewed from brighter lit suburban skies. The distance to 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 ... | 11,412 | zeroshot-train |
Coma Star Cluster [SEP] constellation | Coma Star Cluster
The Coma Star Cluster in Coma Berenices, designated Melotte 111 after its entry in the catalogue of star clusters by P. J. Melotte, is a small but nearby star cluster in our galaxy, containing about 40 brighter stars (magnitude 5 to 10) with a common proper motion. The "Hipparcos" satellite and infrar... | mulberry silk moths.
In 2005, China accounted for 74 percent of the global raw silk production and 90 percent of the world export market.
Industrial plans.
Local governments have and are continuing to introduce new facilities that are expected to bring in latest high-end silk manufacturing machinery that will elevate b... | 11,413 | zeroshot-train |
EGS-zs8-1 [SEP] constellation | EGS-zs8-1
EGS-zs8-1 is a high-redshift Lyman-break galaxy found at the northern constellation of Boötes. In May 2015, EGS-zs8-1 had the highest spectroscopic redshift of any known galaxy, meaning EGS-zs8-1 was the most distant and the oldest galaxy observed. In July 2015, EGS-zs8-1 was surpassed by EGSY8p7 (EGSY-200853... | light travel distance years away. The existence of such early protogalaxies suggests that they must have grown in the so-called "dark ages". As of May 5, 2015, the galaxy EGS-zs8-1 is the most distant and earliest galaxy measured, forming 670 million years after the Big Bang. The light from EGS-zs8-1 has taken 13 billi... | 11,414 | zeroshot-train |
Epsilon Coronae Borealis [SEP] constellation | Epsilon Coronae Borealis
Epsilon Coronae Borealis, Latinized from ε Coronae Borealis, is a multiple star system in the constellation Corona Borealis located around 230 light-years from the Solar System. It shines with a combined apparent magnitude of 4.13, meaning it is visible to the unaided eye in all night skies exc... | 12 September 2016 and it is now so included in the List of IAU-approved Star Names.
In Chinese, (), meaning "Coiled Thong", refers to an asterism consisting of Beta Coronae Borealis, Pi Coronae Borealis, Theta Coronae Borealis, Alpha Coronae Borealis, Gamma Coronae Borealis, Delta Coronae Borealis, Epsilon Coronae Bore... | 11,415 | zeroshot-train |
Eta Centauri [SEP] constellation | Eta Centauri
Eta Centauri, Latinized from η Centauri, is a star in the southern constellation of Centaurus. It has an apparent visual magnitude of +2.35 and is located at a distance of around . In traditional Chinese astronomy, Eta Centauri was known as (meaning: the Second (Star) of "Koo Low").
The stellar classificat... | . The International Variable Star Index lists Eta Centauri as both a Gamma Cassiopeiae variable and a Lambda Eridani variable.
Eta Centauri has about 12 times the mass of the Sun, placing it above the dividing line between stars that evolve into white dwarfs and those that turn into supernovae. It is radiating 8,700 ti... | 11,416 | zeroshot-train |
Eta Serpentis [SEP] constellation | Eta Serpentis
Eta Serpentis (η Ser, η Serpentis) is a star in the constellation Serpens. In particular, it lies in Serpens Cauda, the snake's tail. The star has an apparent visual magnitude of 3.260, making it visible to the naked eye. Parallax measurements give a distance estimate of from the Earth.
This star is large... | ) is represented with the star Eta Serpentis in asterism "Left Wall", Heavenly Market enclosure (see Chinese constellation).
See also.
- Geography of China
- Xihu Trough
- Geography of Japan
- Senkaku Islands (Diaoyu Islands in Chinese)
- Sea of Japan
- South China Sea
Further reading.
- Kim, Suk Kyoon. "China and Japa... | 11,417 | zeroshot-train |
Eyes Galaxies [SEP] constellation | Eyes Galaxies
The Eyes Galaxies (NGC 4435-NGC 4438, also known as Arp 120) are a pair of galaxies about 52 million light-years away in the constellation Virgo. The pair are members of the string of galaxies known as Markarian's Chain.
NGC 4435.
NGC 4435 is a barred lenticular galaxy currently interacting with NGC 4438.... | NGC 1267
NGC 1267 is an elliptical galaxy located about 220 million light-years away in the constellation Perseus. NGC 1267 was discovered by astronomer Heinrich d'Arrest on February 14, 1863. NGC 1267 is a member of the Perseus Cluster and is possibly interacting with the spiral galaxy NGC 1268.
See also.
- List of NG... | 11,418 | zeroshot-train |
F Centauri [SEP] constellation | F Centauri
F Centauri (F Cen) is a star in the constellation Centaurus. It is approximately 490 light years from Earth. F Centauri is a M-type red giant with an apparent magnitude of +5.01. | ), the English, French and Dutch granted what were effectively trade monopolies to joint-stock companies such as the East India Companies and the Hudson's Bay Company.
In the exploration of Africa, there was the proliferation of conflicting European claims to African territory. By the 15th century, Europeans explored t... | 11,419 | zeroshot-train |
Gamma Coronae Australis [SEP] constellation | Gamma Coronae Australis
Gamma Coronae Australis (γ CrA), is a binary star located in the constellation Corona Australis. The system has a combined apparent visual magnitude of 4.20, making it faintly visible to the naked eye. It is located 56.4 light-years (17.3 parsecs) from the Sun, based on its parallax. Gamma Coron... | Blue-white, it is of spectral type B8e. The largest young stars in the region, R, S, T, TY and VV Coronae Australis, are all ejecting jets of material which cause surrounding dust and gas to coalesce and form Herbig–Haro objects, many of which have been identified nearby. Lying adjacent to the nebulosity is the globula... | 11,420 | zeroshot-train |
Gliese 163 [SEP] constellation | Gliese 163
Gliese 163 is an M3.5V red dwarf located 49 light years (15.0pc) from the sun, in the constellation Dorado. Its coordinates in the night sky are RA 04h 9m 16s and Dec. -53°22'. It has a visual magnitude of 11.8 and an absolute magnitude of 10.9. Other stellar catalog names for it include HIP 19394 and LHS 18... | at least
- Gliese 581d, a planet in the star's habitable zone
- Gliese 667, a triple star system in the constellation of Scorpius containing exoplanet GJ 667 Cc in one of the stars' habitable zone
- Gliese 682, a red dwarf in the constellation of Scorpius with two candidate planets, one of which is in the star's habita... | 11,421 | zeroshot-train |
Gliese 317 b [SEP] constellation | Gliese 317 b
Gliese 317 b is an extrasolar planet approximately 50 light-years away in the constellation of Pyxis. The planet was announced in July 2007 to be orbiting the red dwarf star Gliese 317. The planet is a jovian planet that orbits about 95% the distance between Earth to the Sun. Despite of this, it takes abou... | November 13, 2009.
See also.
Other planets that were discovered or confirmed on November 13, 2009:
- HD 34445 b
- HD 126614 Ab
- HD 24496 Ab
- HD 13931 b
- QS Virginis b
Related giant planets around red dwarfs:
- HIP 79431 b
- Gliese 849 b
- Gliese 876 b
- Gliese 876 c
- Gliese 317 b
- Gliese 832 b | 11,422 | zeroshot-train |
Gliese 758 [SEP] constellation | Gliese 758
Gliese 758 is a star in the northern constellation of Lyra. At about magnitude 6 it is a challenge to view with the naked eye even in good seeing conditions, but can be easily seen through a small telescope or binoculars. Parallax measurements from the Hipparcos mission give it an estimated distance of aroun... | 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... | 11,423 | zeroshot-train |
H Scorpii [SEP] constellation | H Scorpii
H Scorpii (H Sco) is a star in the constellation Scorpius. Its apparent magnitude is 4.18. It was initially given the Bayer designation Beta Normae by Lacaille but later moved from Norma to Scorpius.
Located around 343 light-years distant, it shines with a luminosity approximately 576 times that of the Sun an... | AR Cassiopeiae
AR Cassiopeiae (AR Cas) is a multiple star system in the constellation of Cassiopeia. It is thought to be a septuple star system. It is one of only two known star systems with a multiplicity of 7, the other being Nu Scorpii, with no physical multiple stars of greater multiplicity yet found.
Nomenclature.... | 11,424 | zeroshot-train |
HAT-P-3 [SEP] constellation | HAT-P-3
HAT-P-3, is a metal-rich K star located about 450 light-years away in the constellation Ursa Major. At a magnitude of about 11.5 it is not visible to the naked eye but is visible in a small to medium-sized amateur telescope. It is believed to be a relatively young star and has a slightly enhanced level of chrom... | HAT-P-1b
HAT-P-1b is an extrasolar planet orbiting the Sun-like star HAT-P-1, also known as ADS 16402 B. HAT-P-1 is the dimmer component of the ADS 16402 binary star system. It is located roughly 521 light years away from Earth in the constellation Lacerta. HAT-P-1b is among the least dense of any of the known extrasol... | 11,425 | zeroshot-train |
HD 100777 b [SEP] constellation | HD 100777 b
HD 100777 b is an extrasolar planet located approximately 172 light-years away in the constellation of Leo, orbiting the star HD 100777. This is a 1.17 M planet taking 33.15 Ms to orbit at 154.1 Gm or 4.99 μpc from the star at 36% eccentricity. The velocity of the orbit is 29.3 km/s. Dominique Naef discover... | HD 190647
HD 190647 is a yellow subgiant star located approximately 177 light years away in the constellation of Sagittarius. The apparent magnitude is 8 and absolute magnitude is 4. It is also called HIP 99115. In 2007, a planet was found to be orbiting the star.
See also.
- HD 100777
- HD 221287
- List of extrasolar ... | 11,426 | zeroshot-train |
HD 113538 c [SEP] constellation | HD 113538 c
HD 113538 c is an exoplanet approximately 51 light years away from earth in the constellation Centaurus. It orbits its star(HD 113538) once every 1657 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/20130... | 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... | 11,427 | zeroshot-train |
HD 113703 [SEP] constellation | HD 113703
HD 113703, also known as f Centauri (f Cen), is a star in the constellation Centaurus. It is approximately 390 light years from Earth. f Centauri is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.71. | 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-... | 11,428 | zeroshot-train |
HD 118203 [SEP] constellation | HD 118203
HD 118203 is a K-type subgiant star located in the Ursa Major constellation 289 light years away from Earth. It has higher metallicity by 25% and very similar stellar age of 4.6 billion years. It has mass 23% greater than the Sun. It is invisible to the naked eye but it can be seen using binoculars or a teles... | HD 118203 b
HD 118203 b is a jovian planet that takes only 6.13 days or 147 hours to orbit the parent star at a distance of 0.07 astronomical units. It has minimum mass of 2.14 times that of Jupiter but the true mass is not known since inclination is not known. This hot Jupiter is unusual since it has relatively high e... | 11,429 | zeroshot-train |
HD 127726 [SEP] constellation | HD 127726
HD 127726 is a binary star system in the northern constellation of Boötes.
External links.
- HR 5433
- CCDM J14323+2641
- Image HD 127726 | 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-... | 11,430 | zeroshot-train |
HD 128093 [SEP] constellation | HD 128093
HD 128093 is a double star in the constellation Boötes. The brighter component is an F-type main sequence star with a stellar classification of F5V and an apparent magnitude of 6.33. It has a magnitude 11.33 companion at an angular separation of 28.1 along a position angle of 318°.
External links.
- HR 5445
-... | 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-... | 11,431 | zeroshot-train |
HD 140913 [SEP] constellation | HD 140913
HD 140913 is a star very much like our own Sun located in the constellation Corona Borealis (The Northern Crown) 146 light years away.
The space velocity components of this star are = .
Companion.
HD 140913 has a companion called HD 140913 B discovered in 1996. A brown dwarf which is 46 times as massive as Ju... | 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-... | 11,432 | zeroshot-train |
HD 155358 b [SEP] constellation | HD 155358 b
HD 155358 b is a gas giant planet that orbits the star HD 155358, located 142 light years away in the constellation Hercules. This planet orbits at a distance about 63% of distance between Earth and the Sun and has a moderate eccentricity. The planet mass is at least 89% of Jupiter, depending on inclination... | 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... | 11,433 | zeroshot-train |
HD 171238 b [SEP] constellation | HD 171238 b
HD 171238 b is an extrasolar planet which orbits the G-type main sequence star HD 171238, located approximately 164 light years away in the constellation Sagittarius. This planet has minimum mass two and a half times greater than Jupiter and orbits two times closer to the star than Jupiter to the Sun. Howev... | - HD 171238
- List of extrasolar planets | 11,434 | zeroshot-train |
HD 188405 [SEP] constellation | HD 188405
HD 188405 is a binary star in the equatorial constellation of Aquila. The pair have an orbital period of roughly 425 years and an angular separation of 1.085″.
External links.
- CCDM J19553-0644AB
- Image HD 188405 | 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-... | 11,435 | zeroshot-train |
HD 190984 b [SEP] constellation | HD 190984 b
HD 190984 b (also known as HIP 99496 b) is an extrasolar planet which orbits the F-type main sequence star HD 190984, located approximately 330 light years away in the constellation Pavo. This planet is at least three times more massive than Jupiter and takes 13 years and four-and-a-half months to orbit 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 ... | 11,436 | zeroshot-train |
HD 199942 [SEP] constellation | HD 199942
HD 199942 (HR 8038) is an A-type main sequence star in the constellation of Equuleus. At 235.2 light years away, this star shines dimly at an apparent magnitude of 5.98.
Galactic Orbit.
HD 199942 is a double star system, which is moving through the galaxy at a speed of 30.3km/s. Its galactic orbit carry it so... | 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-... | 11,437 | zeroshot-train |
HD 20644 [SEP] constellation | HD 20644
HD 20644 is a star in the constellation Aries. Its apparent magnitude is 4.47. | 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-... | 11,438 | zeroshot-train |
HD 218566 [SEP] constellation | HD 218566
HD 218566 is a star in the equatorial zodiac constellation of Pisces. With an apparent visual magnitude of 8.6, this ninth magnitude star can not be viewed with the naked eye. However, it can be readily seen even with a small telescope.
HD 218566 is a smaller star than the Sun, with about 81% of the Sun's mas... | as and as far as from the Galactic Center. The orbital tilt carries this star as much as from the galactic plane.
Based upon high resolution measurements performed at the W. M. Keck Observatory and analysis performed upon these measurements by amateur astronomer Peter Jalowiczor, HD 218566 shows cyclical variations in ... | 11,439 | zeroshot-train |
HD 23596 [SEP] constellation | HD 23596
HD 23596 is a 7th magnitude star approximately 170 light years away in the constellation Perseus. The visual luminosity of the star is 2.63 times greater than our Sun. HD 23596 dwarfs the Sun is terms of physical properties; including mass, radius, age, metallicity, and temperature. The spectrum of the star is... | 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-... | 11,440 | zeroshot-train |
HD 33283 [SEP] constellation | HD 33283
HD 33283 is an 8th magnitude star in the constellation Lepus. It is located 90 parsecs (294 light years) away from the solar system. HD 33283 is similar to our Sun in terms of spectral type [G4V]. However, the star dwarfs the Sun by 24% more massive, 20% larger, 217 K hotter, and 232% more metals. The star is ... | HD 86081
HD 86081 is a yellow-white dwarf star in the constellation Sextans south of the celestial equator. It is bigger and more massive than our Sun at 1.22 and 1.21 solar units respectively. It has temperature of 6028 K and luminosity of 1.75 solar.
HD 86081 shows no evidence of planetary transits in spite of a 17.6... | 11,441 | zeroshot-train |
HD 37017 [SEP] constellation | HD 37017
HD 37017, also known as V1046 Orionis, is a spectroscopic binary in the equatorial constellation of Orion. The two stars orbit each other with a period of 18.6556 days and an eccentricity of 0.31. The system is part of star cluster NGC 1981.
External links.
- Simbad | 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-... | 11,442 | zeroshot-train |
HD 37124 b [SEP] constellation | HD 37124 b
HD 37124 b is an extrasolar planet approximately 103 light-years away in the constellation of Taurus (the Bull). The planet was discovered in 1999 orbiting the star HD 37124. Based on its mass, it is most likely that this planet is a Jovian planet (like Jupiter). | of Mercury.
Possible class-III planets are HD 37124 b, HD 18742 b, HD 178911 Bb, 55 Cancri c, Upsilon Andromedae c, Kepler-89e, COROT-9b and HD 205739 b. Above 700 K (800 °F, 430 °C), sulfides and chlorides might provide cirrus-like clouds.
Planetary classes Class IV: Alkali metals.
Above 900 K (630 °C/1160 °F), carbon... | 11,443 | zeroshot-train |
HD 52265 b [SEP] constellation | HD 52265 b
HD 52265 b is a gas giant exoplanet located approximately 92 light-years away in the constellation of Monoceros, orbiting the star HD 52265. The planet has a minimum mass slightly more than that of Jupiter. Mean distance between the planet and the star is half that of Earth from the Sun. It was discovered by... | 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... | 11,444 | zeroshot-train |
HD 74156 [SEP] constellation | HD 74156
HD 74156 is a yellow dwarf star (spectral type G0V) in the constellation of Hydra, 210 light years from the Solar System. It is known to be orbited by two giant planets.
Star.
This star is 24% more massive and 64% larger than our Sun. The total luminosity is 2.96 times that of our Sun and its temperature 5960 ... | HD 74156 b
HD 74156 b is an extrasolar planet at least 1.88 times the mass of Jupiter that orbits the star HD 74156. It is most likely a gas giant. This planet was discovered in April 2001 by Dominique Naef and Michel Mayor along with the second planet HD 74156 c. | 11,445 | zeroshot-train |
HD 75289 [SEP] constellation | HD 75289
HD 75289 is a 6th magnitude star in the constellation of Vela. Like our Sun, it is a yellow dwarf but slightly more massive, hotter and luminous. The spectral type of the star is G0 V. Under exceptionally good circumstances it might be visible to the unaided eye; however, usually binoculars are needed.
In 2004... | . This planet is a typical hot Jupiter that takes only about 3.51 days to revolve at an orbital distance of 0.0482 AU.
HD 75289 B.
HD 75289 B is a possible red dwarf star orbiting HD 75289. The stars share the same proper motion so they are probably related. Apparent distance between the two stars is about 21.5 arcseco... | 11,446 | zeroshot-train |
HD 78004 [SEP] constellation | HD 78004
HD 78004 (c Vel, c Velorum) is a star in the constellation Vela.
HD 78004 is an orange K-type giant with an apparent magnitude of +3.75. It is approximately 300 light years from Earth. | C Velorum
The Bayer designations c Velorum and C Velorum are distinct. Due to , both designations link here. For the star
- c Velorum, see HD 78004 (HR 3614)
- C Velorum, see HD 73155 (HR 3407)
See also.
- γ Velorum (Gamma Velorum) | 11,447 | zeroshot-train |
HD 81101 [SEP] constellation | HD 81101
HD 81101, also known as k Carinae (k Car), is a star in the constellation Carina.
k Carinae is a yellow G-type giant with an apparent magnitude of +4.79. It is approximately 223 light years from Earth. | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,448 | zeroshot-train |
HD 90156 b [SEP] constellation | HD 90156 b
HD 90156 b is an extrasolar planet which orbits the G-type main sequence star HD 90156, located approximately 73 light years away. | 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... | 11,449 | zeroshot-train |
HD 9446 b [SEP] constellation | HD 9446 b
HD 9446 b is an exoplanet discovered in 2010 orbiting the star HD 9446 in the constellation Triangulum, 50 parsecs from Earth.
See also.
- HD 9446 c | period of 267 days. It is a red giant of spectral type M3.5-8e, lying around 960 light-years away. HD 12545, also known as XX Trianguli, is
an orange giant of spectral type K0III around 520 light-years distant with a visual magnitude of 8.42. A huge starspot larger than the diameter of the sun was detected on its surfa... | 11,450 | zeroshot-train |
HR 3082 [SEP] constellation | HR 3082
HR 3082 is a double star in the northern circumpolar constellation of Camelopardalis. It is faintly visible to the naked eye with an apparent visual magnitude of 5.39. The system is moving closer to the Sun with a heliocentric radial velocity of +2.7 km/s. It is currently at a distance of around 323 light years... | HR 4458
HR 4458 is a binary star system in the equatorial constellation of Hydra. It has the Gould designation 289 G. Hydrae; "HR 4458" is the Bright Star Catalogue designation. At a distance of 31.13 light years, it is the closest star system to the solar system within this constellation. This object is visible to the... | 11,451 | zeroshot-train |
IC 2177 [SEP] constellation | IC 2177
IC 2177 is a region of nebulosity that lies along the border between the constellations Monoceros and Canis Major. It is a roughly circular H II region centered on the Be star HD 53367. This nebula was discovered by Welsh amateur astronomer Isaac Roberts and was described by him as "pretty bright, extremely lar... | was catalogued as part of the major clustering of reflection nebula as CMa R1 by van den Bergh in 1966. Reflection nebulas were identified on blue plates of the Palomar Sky Survey, with positive confirmation made by checking nebulosity on the red plates. It was again later catalogued as LBN 1037 or LBN 225.27-02.42
See... | 11,452 | zeroshot-train |
IC 289 [SEP] constellation | IC 289
IC 289 is a planetary nebula in the constellation Cassiopeia. It was discovered by Lewis Swift in early September 1888. It lies close to the 10th magnitude star BD +60° 0631. N.J. Martin described IC 289 as "A nice, faint round planet like planetary nebula. The uniform oval disc shows some irregularity in bright... | NGC 499
NGC 499, also occasionally referred to as PGC 5060, IC 1686 or GC 289, is a lenticular galaxy in the constellation Pisces. It located approximately 197 million light-years from the Solar System and was discovered on 12 September, 1784 by astronomer William Herschel.
The NGC 499 Group is named after the galaxy.
... | 11,453 | zeroshot-train |
IC 3418 [SEP] constellation | IC 3418
IC 3418 is a galaxy that is most well noted for its tidal tail, which formed after the galaxy collided with the Virgo Cluster some 54 million light years from Earth. The galaxy is home to many starburst regions.
The galaxy is thought to be evolving from a dwarf irregular galaxy into a dwarf elliptical galaxy, a... | SDSS J1229+1122
SDSS J1229+1122 (SDSS J122952.66+112227.8) is a blue supergiant O-type star in the tail of dwarf irregular galaxy IC 3418. It illuminates a nebula clump of gas, and was discovered from the spectrum of the illumination source. The clump of gas resides in a tail caused by ram pressure stripping of gas fro... | 11,454 | zeroshot-train |
IC 4970 [SEP] constellation | IC 4970
IC 4970 is an unbarred lenticular galaxy of type "" in the constellation Pavo. It is from Earth and is interacting with the barred spiral galaxy . It was discovered on 21 September 1900 by American astronomer DeLisle Stewart.
Interaction with NGC 6872.
IC 4970 is located a few arcseconds away from the much larg... | hundred million years. Star formation rates in the northeast extended arm are twice that of the southwest extended arm, and five times the formation rate in the sections of the arms closer to the central region.
Interaction with IC 4970.
IC 4970 is a nearby lenticular galaxy, located only a few arcseconds away, and is ... | 11,455 | zeroshot-train |
Kappa Arietis [SEP] constellation | Kappa Arietis
Kappa Arietis, Latinized from κ Arietis, is the Bayer designation for a binary star in the northern constellation of Aries. It is approximately distant from Earth. The combined apparent visual magnitude of the pair is 5.02, making the system bright enough for it to be dimly visible to the naked eye. Kappa... | freedom. He has been coy about whether he is a member of any paramilitary organisation, however, suspicions were raised when he was seen leaving a farmhouse in rural Co. Fermanagh with well known members of the INLA.
Playing career.
Playing career Club.
McGrath plays his club hurling with Kilmacud Crokes and has enjoye... | 11,456 | zeroshot-train |
Kappa Fornacis [SEP] constellation | so the components of the secondary are the source of the excess energy in the system.
Properties.
In terms of an object on the celestial sphere, Kappa Fornacis is a fifth magnitude star that lies close to the border between the northerly border of Fornax with Cetus. At magnitude 5.2, it is approximately the seventh-bri... | Kappa Fornacis
Kappa Fornacis (κ For) is a star system that lies approximately 72 light-years away. The system consists of a somewhat evolved primary orbited by a massive, 'dark' secondary that is actually itself a close red dwarf binary, making a hierarchal triple system.
Multiplicity.
Kappa Fornacis was found to be 0... | 11,457 | zeroshot-train |
Kepler-69 [SEP] constellation | Kepler-69
Kepler-69 ("KOI-172", "2MASS J19330262+4452080", "KIC 8692861") is a G-type main-sequence star similar to the Sun in the constellation Cygnus, located about from Earth. On April 18, 2013 it was announced that the star has two planets. Although initial estimates indicated that the terrestrial planet Kepler-69c... | 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... | 11,458 | zeroshot-train |
Lambda Pegasi [SEP] constellation | Lambda Pegasi
Lambda Pegasi (λ Peg, λ Pegasi) is a fourth-magnitude star in the constellation Pegasus.
λ Pegasi is a yellow giant with stellar classification G8II-III. With a mass of and radius that is , the star boasts a bolometric luminosity that is roughly . Its apparent magnitude was calibrated in 1983 at 3.96, yie... | distance of its line-of-sight double μ Pegasi.
In the constellation, Lambda and Mu lie to the southwest of Beta Pegasi, the nearest bright star. | 11,459 | zeroshot-train |
Luyten 726-8 [SEP] constellation | Luyten 726-8
Luyten 726-8, also known as Gliese 65, is a binary star system that is one of Earth's nearest neighbors, at about 8.7 light years from Earth in the constellation Cetus. Luyten 726-8B is also known under the variable star designation UV Ceti, being the archetype for the class of flare stars.
Star system.
Th... | Luyten (disambiguation)
Willem Jacob Luyten (1899–1994) was a Dutch-American astronomer.
Luyten may also refer to:
- Luyten (surname), with a list of other people with the surname Luyten
- 1964 Luyten, an asteroid named after Willem Jacob Luyten
- Luyten's Star, a red dwarf in the constellation Canis Minor
- Luyten b (... | 11,460 | zeroshot-train |
MOA-2008-BLG-310Lb [SEP] constellation | MOA-2008-BLG-310Lb
MOA-2008-BLG-310Lb is an extrasolar planet which orbits probably the late K-type star MOA-2008-BLG-310L, located at least 20000 light years away in the constellation Scorpius. This planet has mass 23% of Jupiter or 77% of Saturn and orbits at 1.25 AU from the star. This planet was discovered by using... | extrasolar planets.
Planets discovered.
μFUN played an important role in discovery and analysis of the following extrasolar planets:
- OGLE-2005-BLG-071Lb
- OGLE-2005-BLG-071Lb
- OGLE-2005-BLG-169Lb
- OGLE-2006-BLG-109Lb, OGLE-2006-BLG-109Lc
- MOA-2007-BLG-400Lb
- MOA-2008-BLG-310Lb
- MOA-2009-BLG-387Lb
- MOA-2009-BLG-... | 11,461 | zeroshot-train |
Messier 28 [SEP] constellation | Messier 28
Messier 28 or M28, also known as NGC 6626, is a globular cluster of stars in the constellation Sagittarius. It was discovered by French astronomer Charles Messier on July 27, 1764. He briefly described it as a "nebula containing no star... round, seen with difficulty in 3½-foot telescope; Diam 2′." The 2′ at... | 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... | 11,462 | zeroshot-train |
Messier 47 [SEP] constellation | Messier 47
Messier 47 (M47 or NGC 2422) is an open cluster in the constellation Puppis. It was discovered by Giovanni Batista Hodierna before 1654 and independently discovered by Charles Messier on February 19, 1771. It was later independently discovered again, under the current name NGC 2422.
There is actually no clus... | Messier 77
Messier 77 or M77, also known as NGC 1068, is a barred spiral galaxy about 47 million light-years away in the constellation Cetus. Messier 77 was discovered by Pierre Méchain in 1780, who originally described it as a nebula. Méchain then communicated his discovery to Charles Messier, who subsequently listed ... | 11,463 | zeroshot-train |
Messier 85 [SEP] constellation | Messier 85
Messier 85 (also known as M85 or NGC 4382 or PGC 40515 or ISD 0135852) is a lenticular galaxy, or elliptical galaxy for other authors, in the Coma Berenices constellation. It is 60 million light-years away, and it is estimated to be 125,000 light-years across.
It was discovered by Pierre Méchain in 1781. It ... | M59
M59 may refer to:
- Messier 59, an elliptical galaxy in the constellation Virgo
- M59 (APC), a United States military vehicle
- M59 rifle, a Yugoslav copy of the SKS
- M-59 (Michigan highway), a Michigan state highway near Detroit
- "Meridian 59", an online game
- M59/85, a Yugoslav modification of Stahlhelm that e... | 11,464 | zeroshot-train |
Mu Aquarii [SEP] constellation | Mu Aquarii
Mu Aquarii, Latinized from μ Aquarii, is the Bayer designation for a binary star system in the equatorial constellation of Aquarius. It is visible to the naked eye with a combined apparent visual magnitude of 4.7. Based upon parallax measurements, the distance to this system is about . Mu Aquarii is a spectr... | 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... | 11,465 | zeroshot-train |
NGC 11 [SEP] constellation | NGC 11
NGC 11 is a spiral galaxy located in the Andromeda constellation. It is located at right ascension ; declination ; under J2000.0 coordinates and was discovered by Édouard Stephan on October 24 1881. | NGC 805
NGC 805 is a lenticular galaxy approximately 194 million light-years away from Earth in the constellation of Triangulum. It was discovered by German astronomer Heinrich Louis d'Arrest on September 26, 1864 with the 11-inch refractor at Copenhagen.
See also.
- Lenticular galaxy
- List of NGC objects (1–1000)
- ... | 11,466 | zeroshot-train |
NGC 129 [SEP] constellation | NGC 129
NGC 129 is an open cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1788. It is located almost exactly halfway between the bright stars Caph (β Cassiopeiae) and γ Cassiopeiae. It is large but not dense and can be observed by binoculars, where the most obvious is a small triangle... | NGC 4349
NGC 4349 is an open cluster in the constellation Crux. It was discovered by James Dunlop in 1826. It is located approximately 7,000 light years away from Earth.
Characteristics.
There are 390 probable member stars within the angular radius of the cluster and 129 within the central part of the cluster. The tida... | 11,467 | zeroshot-train |
NGC 1333 [SEP] constellation | NGC 1333
NGC 1333 is a reflection nebula located in the constellation Perseus. It belongs to the Perseus molecular cloud.
In 2011 researchers reported finding 30 to 40 brown dwarf objects in the cloud and in the Rho Ophiuchi cloud complex.
It was discovered by the SPITZER space telescope.
External links.
- Agrupació As... | 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... | 11,468 | zeroshot-train |
NGC 1788 [SEP] constellation | NGC 1788
NGC 1788 is a reflection nebula in the constellation of Orion. It is rather sharply defined on its southwest perimeter where it is flanked by the dark nebula known as Lynds 1616. Lynds 1616 is apparently part of NGC 1788. The brightest involved star is 10th magnitude and lies in the northwest sector.
External ... | NGC 2500
NGC 2500 is a barred spiral galaxy in the constellation Lynx which was discovered by William Herschel in 1788. Much like the local group in which our own Milky Way galaxy is situated, NGC 2500 is part of NGC 2841 group of galaxies which also includes NGC 2541, NGC 2537 and NGC 2552. It has a H II nucleus and e... | 11,469 | zeroshot-train |
NGC 1931 [SEP] constellation | NGC 1931
NGC 1931, is an emission and reflection nebula in the constellation Auriga. The nebula has been referred to as a "miniature version of the Orion Nebula", as it shares some of the same characteristics. It is a mixed emission-reflection nebula, and contains a smaller version of the Trapezium in its hot young sta... | 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... | 11,470 | zeroshot-train |
NGC 2080 [SEP] constellation | NGC 2080
NGC 2080 (The "Ghost Head Nebula") is a star-forming region and emission nebula to the south of the 30 Doradus (Tarantula) nebula, in the southern constellation Dorado. It belongs to the Large Magellanic Cloud, a satellite galaxy to the Milky Way, which is at a distance of 168,000 light years. NGC 2080 was dis... | of light, it appears blue, as in the area surrounding A1 and A2.
NGC 2080 should not be confused with the Ghost Nebula (Sh2-136) or the Little Ghost Nebula (NGC 6369).
See also.
- Emission nebula
- List of NGC objects (2001–3000)
- Large Magellanic Cloud
External links.
- SEDS
- Hubble Sends Season's Greetings from the... | 11,471 | zeroshot-train |
NGC 2516 [SEP] constellation | NGC 2516
NGC 2516 is an open star cluster in the southern sky in the constellation Carina discovered by Abbe Lacaille in 1751-1752. It is also called Southern Beehive or the Sprinter.
Description.
This bright cluster itself is easily visible with the naked eye as a hazy patch, but is resolvable into stars using binocul... | a prime supernova candidate for the next several hundred thousand years because it has reached the end of its estimated million-year life span.
NGC 2516 is an open cluster that is both quite large (approximately half a degree square) and bright, visible to the unaided eye. It is located 1100 light-years from Earth and ... | 11,472 | zeroshot-train |
NGC 2812 [SEP] constellation | NGC 2812
NGC 2812 is a lenticular galaxy in the constellation Cancer. It was discovered by Albert Marth on February 17, 1865. | 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... | 11,473 | zeroshot-train |
NGC 2818 [SEP] constellation | NGC 2818
NGC 2818 is a planetary nebula located in the southern constellation Pyxis (The Compass). It consists largely of glowing gases from the star's outer layers ejected during the final stages of its life when it had run out of the fuel necessary to sustain its core fusion processes. The remnants of its core will r... | NGC 2438
NGC 2438 is a planetary nebula about 3,000 light years away in the constellation Puppis. It was discovered by William Herschel on March 19, 1786.
NGC 2438 appears to lie within the cluster M46, but it is most likely unrelated since it does not share the cluster's radial velocity. The case is yet another exampl... | 11,474 | zeroshot-train |
NGC 3079 [SEP] constellation | NGC 3079
NGC 3079 is a barred spiral galaxy about 50 million light-years away, and located in the constellation Ursa Major. A prominent feature of this galaxy is the "bubble" forming in the very center (see picture below). The Supermassive black hole at the core has a mass of .
Center Bubble.
The bubble forming in the ... | black hole is listed as fourth largest, and it is unusually large in proportion to the host galaxy, being 14% of the mass, instead of the usual 0.1%
- NGC 1566
- NGC 2778
- NGC 2787
- NGC 3079
- NGC 3115
- NGC 3245
- NGC 3377
- NGC 3384
- NGC 3608
- NGC 3894
- NGC 3998
- NGC 4151
- NGC 4261
- NGC 4291
- NGC 4342
- NGC ... | 11,475 | zeroshot-train |
NGC 3260 [SEP] constellation | NGC 3260
NGC 3260 is an elliptical galaxy in the constellation Antlia. It is a member of the Antlia Cluster, which lies about away. | 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... | 11,476 | zeroshot-train |
NGC 346 [SEP] constellation | NGC 346
NGC 346 is an open cluster with associated nebula located in the Small Magellanic Cloud that appears in the constellation Tucana. It contains HD 5980, the brightest star in the SMC.
External links.
- ESA
- Hubble Heritage site Hubble picture and information on NGC 346
- ESO Beautiful Image of a Cosmic Sculpture | 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... | 11,477 | zeroshot-train |
NGC 4203 [SEP] constellation | NGC 4203
NGC 4203 is the "New General Catalogue" identifier for a lenticular galaxy in the northern constellation of Coma Berenices. It was discovered on March 20, 1787 by English astronomer William Herschel, and is situated 5.5° to the northwest of the 4th magnitude star Gamma Comae Berenices and can be viewed with a ... | , NGC 4173, NGC 4203, NGC 4245, NGC 4251, NGC 4274, NGC 4283, NGC 4310, NGC 4314, NGC 4359, NGC 4414, NGC 4509, and NGC 4525. Another survey placed NGC 4278 in the same group with NGC 4631, NGC 4656, NGC 4559, NGC 4448, and NGC 4414. It is part of the Coma I Group which is part of the Virgo Supercluster.
NGC 4283 lies ... | 11,478 | zeroshot-train |
NGC 467 [SEP] constellation | NGC 467
NGC 467 is an elliptical galaxy in the constellation Pisces. It was discovered on 8 October 1785 by William Herschel.
See also.
- List of NGC objects (1–1000)
External links.
- NGC 467 at spider.seds.org
- NGC 467 at WikiSky | 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... | 11,479 | zeroshot-train |
NGC 49 [SEP] constellation | NGC 49
NGC 49 is a lenticular galaxy in the Andromeda constellation. The galaxy was discovered by the American astronomer Lewis A. Swift on September 7, 1885. | NGC 50
NGC 50 is an elliptical galaxy in the constellation Cetus with a diameter of 170,000 light-year's. It was discovered in 1865 by Gaspare Ferrari. The galaxy is, in comparison to the Milky Way, about 1.5-2 times as large. It is also physically close to NGC 49.
Other names for NGC 50 are MCG -1-1-58 and PGC 983.
Se... | 11,480 | zeroshot-train |
NGC 5161 [SEP] constellation | NGC 5161
NGC 5161 is a spiral galaxy in the constellation Centaurus.
See also.
- New General Catalogue
External links.
- detailed information on NGC 5161 | 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... | 11,481 | zeroshot-train |
NGC 5248 [SEP] constellation | NGC 5248
NGC 5248 (also known as Caldwell 45) is a compact intermediate spiral galaxy about 59 million light-years away in the constellation Boötes. It is a member of the NGC 5248 Group of galaxies, itself one of the Virgo III Groups strung out to the east of the Virgo Supercluster of galaxies. Distance measurements to... | / 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... | 11,482 | zeroshot-train |
NGC 5371 [SEP] constellation | NGC 5371
NGC 5371 is a face-on spiral galaxy in the constellation Canes Venatici. NGC 5371 (which also seems to be known as NGC 5390) is a symmetrical face-on Sbc barred spiral galaxy at a distance of 100 million light years. This galaxy with Hickson Galaxy Group 68 makes up the Big Lick Galaxy Group. | 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... | 11,483 | zeroshot-train |
NGC 5544 [SEP] constellation | NGC 5544
NGC 5544 is a barred spiral galaxy in the constellation Boötes. It is interacting with spiral galaxy NGC 5545.
External links.
- Image NGC 5544
- http://seds.org/
- Distance | spiral arms that are described as "filaments" by Arp.
List of galaxies in the catalog Amorphous galaxies Galaxies with material ejected from nuclei.
The ejecta in many of these objects appear to be tidal features created by gravitational interactions. In some cases (such as for NGC 5544 and NGC 5545 in Arp 199), the "e... | 11,484 | zeroshot-train |
NGC 5653 [SEP] constellation | NGC 5653
NGC 5653 is a spiral galaxy in the constellation Boötes.
External links.
- HubbleSite NewsCenter: NGC 5653
References.
- IRAS F14280+3126
- http://hubblesite.org/ | of spiral galaxy) of magnitude 10.2. It measures 6.5 by 4.9 arcminutes. Fifty million light-years from Earth, NGC 5248 is a member of the Virgo Cluster of galaxies; it has dim outer arms and obvious H II regions, dust lanes, and young star clusters. NGC 5676 is another type Sc galaxy of magnitude 10.9. It measures 3.9 ... | 11,485 | zeroshot-train |
NGC 6124 [SEP] constellation | NGC 6124
NGC 6124 is an open cluster located 18,600 light years away in the constellation Scorpius. It was discovered by Abbe Lacaille in 1751 during his South African tour.
The cluster is large and bright, with about 125 stars visible.
External links.
- NGC 6124 at Messier45 | 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... | 11,486 | zeroshot-train |
NGC 6401 [SEP] constellation | NGC 6401
NGC 6401 is a globular cluster in the constellation Ophiuchus. William Herschel discovered this star cluster in 1784 with his 47 cm telescope, but mistakenly believed it to be a bright nebula. Later his son, John Herschel, was to make the same error because the technology of the day was insufficient to allow t... | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,487 | zeroshot-train |
NGC 6723 [SEP] constellation | NGC 6723
NGC 6723 is a globular cluster in the constellation Sagittarius. Its magnitude is given between 6 and 6.8, and diameter between 7 and 11 arcminutes, class VII with stars magnitude 14 and dimmer. It is near the border of Sagittarius and Corona Australis.
References.
- Robert Burnham, Jr, "Burnham's Celestial Ha... | globular cluster, NGC 6723, in the Milky Way's galactic halo
- 740 million years: 47 Tucanae, second-brightest globular cluster in the Milky Way, forms
- 750 million years: Galaxy IOK-1 a Lyman alpha emitter galaxy, forms. GN-108036 forms—galaxy is 5 times larger and 100 times more massive than the present day Milky Wa... | 11,488 | zeroshot-train |
NGC 6752 [SEP] constellation | NGC 6752
NGC 6752 (also known as Caldwell 93) is a globular cluster in the constellation Pavo. It is the third-brightest in the sky, after Omega Centauri and 47 Tucanae, and is best seen from June to October in the Northern Hemisphere.
NGC 6752 was first identified by one James Dunlop of Parramatta on 30 June 1826, who... | forms
- 2.02 billion years (11.78 Gya): Messier 62 forms – contains high number of variable stars (89) many of which are RR Lyrae stars.
- 2.2 billion years (11.6 Gya): Globular Cluster NGC 6752, third-brightest, forms in Milky Way
- 2.4 billion years (11.4 Gya): Quasar PKS 2000-330 forms.
- 2.41 billion years (11.39 G... | 11,489 | zeroshot-train |
NGC 6822 [SEP] constellation | NGC 6822
NGC 6822 (also known as Barnard's Galaxy, IC 4895, or Caldwell 57) is a barred irregular galaxy approximately 1.6 million light-years away in the constellation Sagittarius. Part of the Local Group of galaxies, it was discovered by E. E. Barnard in 1884 (hence its name), with a six-inch refractor telescope. It ... | -like nebula N70 in the LMC.
See also.
- Bubble Nebula (NGC 6822)
- NGC 6822
External links.
- Simbad
- Clayton, C.A. "The Dynamics of the giant ring nebula Hubble III in NGC 6822", "Monthly Notices of the Royal Astronomical Society", vol. 226, May 15, 1987, p. 493-504 | 11,490 | zeroshot-train |
NGC 79 [SEP] constellation | NGC 79
NGC 79 is an elliptical galaxy estimated to be about 240 million light-years away in the constellation of Andromeda. Its apparent magnitude is 14.9. It was descovered on 14 November 1884 by Guillaume Bigourdan. | NGC 3201
NGC 3201 (also known as Caldwell 79) is a low galactic latitude globular cluster in the southern constellation of Vela. It has a very low central concentration of stars. This cluster was discovered by James Dunlop on May 28, 1826 and listed it in his 1827 catalogue. He described it as "a pretty large pretty br... | 11,491 | zeroshot-train |
NGC 891 [SEP] constellation | NGC 891
NGC 891 (also known as Caldwell 23 or Silver Sliver Galaxy) is an edge-on unbarred spiral galaxy about 30 million light-years away in the constellation Andromeda. It was discovered by William Herschel on October 6, 1784. The galaxy is a member of the NGC 1023 group of galaxies in the Local Supercluster. It has ... | In 1999, the Hubble Space Telescope imaged NGC 891 in infrared.
In 2005, due to its attractiveness and scientific interest, NGC 891 was selected to be the first light image of the Large Binocular Telescope.
In 2012, it was again used as a first light image of the Discovery Channel Telescope with the Large Monolithic Im... | 11,492 | zeroshot-train |
NGC 925 [SEP] constellation | NGC 925
NGC 925 is a barred spiral galaxy located about 30 million light-years away in the constellation Triangulum. The morphological classification of this galaxy is SB(s)d, indicating that it has a bar structure and loosely wound spiral arms with no ring. The spiral arm to the south is stronger than the northern arm... | spiral arm and the offset bar—are typically characteristics of a Magellanic spiral galaxy. The galaxy is inclined at an angle of 55° to the line of sight along a position angle of 102°.
The galaxy is a member of the NGC 1023 Group, a nearby, gravitationally-bound group of galaxies associated with NGC 1023. However, the... | 11,493 | zeroshot-train |
Nova Sagittarii 1898 [SEP] constellation | Nova Sagittarii 1898
Nova Sagittarii 1898 (also called V1059 Sagittarii) was a nova, which lit up in 1898 in the constellation Sagittarius. Nova Sagittarii 1898 reached magnitude 4.5.
External links.
- https://web.archive.org/web/20050912175943/http://www.tsm.toyama.toyama.jp/curators/aroom/var/nova/1600.htm | Variable Stars using the GCVS format for the naming of variable stars. When more than one nova is discovered in a constellation in one year, a numeric suffix is appended; hence "Nova Sagittarii 2011 #2", "Nova Sagitarii 2011 #3", etc.
See also.
- Nova
- List of supernovae
- Variable star
External links.
- CBAT List of ... | 11,494 | zeroshot-train |
OGLE-TR-56b [SEP] constellation | OGLE-TR-56b
OGLE-TR-56b is an extrasolar planet located approximately 1500 parsecs away in the constellation of Sagittarius, orbiting the star OGLE-TR-56. This planet was the first known exoplanet to be discovered with the transit method. The object was discovered by the OGLE project, announced on July 5, 2002 and conf... | ). But unlike it, the planet has a radius comparable to Jupiter which is typical to other transiting planets detected by OGLE. However, those other planets tend to be more massive and orbit even closer than typical hot Jupiters. Therefore, this planet is an important "missing link" between the different types of transi... | 11,495 | zeroshot-train |
R Corvi [SEP] constellation | R Corvi
R Corvi (R Crv) is a Mira variable star in the constellation Corvus, which ranges from a magnitude of 6.7 to 14.4 with a period of approximately 317 days. In the sky it appears close to Gamma Corvi and can be seen in the same binocular field. Extrapolating its luminosity from its period of 317 days yields a dis... | the silverware.
Achievements.
- All India Rural Sports Tournament 2007–2008
- National School Championship 2010–2011
- Kerala Junior National Football Championship 2009–2010
- South Zone University Championship 2012–2013 (Calicut University)
- South Zone University Championship 2013–2014 (Calicut University)
- All Indi... | 11,496 | zeroshot-train |
R Monocerotis [SEP] constellation | R Monocerotis
R Monocerotis (R Mon) is a T Tauri variable in the constellation Monoceros. The apparent magnitude of R Mon varies between 10 and 12 and the spectral type B8IIIe.
The star is located in a diffuse nebula called "Hubble's Variable Nebula" (NGC 2261). According to some astronomers, the "star" R Monocerotis i... | 11,497 | zeroshot-train | |
R Reticuli [SEP] constellation | R Reticuli
R Reticuli (R Ret) is a Mira variable star in the constellation Reticulum. It varies between magnitudes 6.35 and 14.2 over a period of 281 days. Although this star was also assigned the variable star designation "S Reticuli", this designation is no longer in use. | two albums were recorded at Pachyderm Studios. Songs from the second album were featured on NPR, and Baeble Music. Their subsequent single release, "Death Cap" and its accompanying music video, which was filmed in Iceland, was featured in "Paste Magazine".
After graduating from the University of Minnesota with a degree... | 11,498 | zeroshot-train |
Rho Aquarii [SEP] constellation | Rho Aquarii
Rho Aquarii, Latinized from ρ Aquarii, is the Bayer designation for a binary star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of +5.34. Based upon parallax measurements made during the Hipparcos mission, this star is at a distance of roughly ... | Aquarii and Rho Aquarii. Consequently, the Chinese name for Theta Aquarii itself is (, ). Possibly, the name "Lei", meaning "tears (weeping)" in Chinese, derives from the Chinese name for this star.
Properties.
Ancha belongs to the spectral class G8 with a luminosity class of III–IV suggesting that, at an age of 437 mi... | 11,499 | zeroshot-train |
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