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Barnard 68 [SEP] constellation | Barnard 68
Barnard 68 is a molecular cloud, dark absorption nebula or Bok globule, towards the southern constellation Ophiuchus and well within our own galaxy at a distance of about 400 light-years, so close that not a single star can be seen between it and the Sun. American astronomer Edward Emerson Barnard added this... | Though it is currently stable, Barnard 68 will eventually collapse, inciting the process of star formation. One unusual feature of Barnard 68 is its vibrations, which have a period of 250,000 years. Astronomers speculate that this phenomenon is caused by the shock wave from a supernova.
Voyager 1 is in the same directi... | 11,600 | zeroshot-train |
Chi Aquarii [SEP] constellation | Chi Aquarii
Chi Aquarii, Latinized from χ Aquarii, is the Bayer designation of a star in the equatorial constellation of Aquarius. The distance to this star, based upon parallax measurements with a 7% margin of error, is roughly . It is visible to the naked eye with an apparent visual magnitude of +5.06.
This is a red ... | 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... | 11,601 | zeroshot-train |
Chi Sagittarii [SEP] constellation | Chi Sagittarii
The Bayer designation Chi Sagittarii (χ Sagittarii) is shared by three star systems in the zodiac constellation of Sagittarius. The brightest of these, χ Sagittarii and χ Sagittarii, are separated by 0.56° on the sky. The dimmer star χ Sagittarii is located between them, 0.10° from χ, and is too faint to... | . "Montuno"
18. "Tradición"
19. "Everlasting Love"
20. Ballad Medley: "Cuts Both Ways" / "I See Your Smile" / "Words Get in the Way" / "Can't Stay Away from You"
21. "Always Tomorrow"
22. "Coming Out of the Dark"
23. "I'm Not Giving You Up"
24. "Show Me the Way Back to Your Heart"
25. "Abriendo Puertas" | 11,602 | zeroshot-train |
Delta Trianguli [SEP] constellation | Delta Trianguli
Delta Trianguli (Delta Tri, δ Trianguli, δ Tri) is a spectroscopic binary star system approximately away in the constellation of Triangulum. The primary star is a yellow dwarf, while the secondary star is thought to be an orange dwarf. It has an apparent magnitude of +4.87 and forms an optical (line-of-... | by the manner in which they adjust Date1 and/or Date2 for the end of the month. Each convention has a set of rules directing the adjustments.
Treating a month as 30 days and a year as 360 days was devised for its ease of calculation by hand compared with manually calculating the actual days between two dates. Also, bec... | 11,603 | zeroshot-train |
EK Trianguli Australis [SEP] constellation | EK Trianguli Australis
EK Trianguli Australis is a star in the constellation Triangulum Australe. It is a dwarf nova of the SU Ursae Majoris type that officially classified as such in 1980, after the characteristic eruptions of a short eruption and a supereruption were observed in May 1978 and June 1979 respectively. T... | to rename the airport "Appleton International Airport." The new name was officially implemented in 2015 on August 21, during the golden anniversary celebration of the airport.
Facilities.
The airport covers at an elevation of above sea level. It has 2 concrete runways:
- Runway 3/21: 8,002 x 150 ft (2,439 x 46 m.), Sur... | 11,604 | zeroshot-train |
Epsilon Corvi [SEP] constellation | Epsilon Corvi
Epsilon Corvi (ε Crv, ε Corvi) is a star in the southern constellation of Corvus. It has the traditional name Minkar , from Arabic منقار "minqar" meaning "beak [of the crow]" The apparent visual magnitude is +3.0 and it is located at a distance of from Earth.
In Chinese, (), meaning "Chariot (asterism)", ... | Zeta Crateris
Zeta Crateris (ζ Crateris) is a probable binary star system in the southern constellation of Crater. Zeta Crateris appears to be about half-way between Epsilon Corvi to the southeast and Beta Crateris to the northwest, and marks the lower left corner of the rim of the bowl. Eta Crateris lies somewhat less... | 11,605 | zeroshot-train |
Gamma Phoenicis [SEP] constellation | Gamma Phoenicis
Gamma Phoenicis is a star system in the constellation Phoenix, located around distant.
γ Phoenicis is a spectroscopic binary and a small amplitude variable star. The star system shows regular variations in brightness that were reported as a 97.5 day period in the Hipparcos catalogue, but have since been... | of the equator. It is most visible from locations such as Australia and South Africa during late Southern Hemisphere spring. Most of the constellation lies within, and can be located by, forming a triangle of the bright stars Achernar, Fomalhaut and Beta Ceti—Ankaa lies roughly in the centre of this.
Features.
Features... | 11,606 | zeroshot-train |
HD 102272 b [SEP] constellation | HD 102272 b
HD 102272 b is an extrasolar planet approximately 1,200 light-years away in the constellation of Leo. The planet was discovered orbiting the K-type giant star HD 102272 in 2008. The planet was discovered by the radial velocity method, using the Hobby-Eberly Telescope. Another planet, HD 102272 c, was also d... | have at least 2.6 times the mass of Jupiter.
See also.
- HD 102272 b | 11,607 | zeroshot-train |
HD 111915 [SEP] constellation | HD 111915
HD 111915, also known by the Bayer designation e Centauri (e Cen), is a star in the constellation Centaurus.
e Centauri is an orange K-type giant with an apparent magnitude of +4.33. It is approximately 294 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-... | 11,608 | zeroshot-train |
HD 114386 [SEP] constellation | HD 114386
HD 114386 is a 9th magnitude star located approximately 91 light years away in the constellation of Centaurus. It is an orange dwarf, and rather dim compared to our Sun. To see it, one needs a telescope or good binoculars.
In 2004, the Geneva Extrasolar Planet Search Team announced the discovery of an extraso... | HD 114783
HD 114783 is an 8th magnitude star about 66.9 light years away in the constellation of Virgo. As an orange dwarf it is somewhat dimmer and cooler than our Sun. The spectral type of the star is K0V. The star is not visible with the unaided eye, but is easy target for binoculars.
In 2001, the California and Car... | 11,609 | zeroshot-train |
HD 131473 [SEP] constellation | HD 131473
HD 131473 is a binary star system in the northern constellation of Boötes. The primary is an F-type subgiant with a stellar classification of F4IV, while its companion is a G-type subgiant with a stellar classification of G1IV.
External links.
- HR 5550
- Image HD 131473
- CCDM J14534+154 | 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-... | 11,610 | zeroshot-train |
HD 136118 b [SEP] constellation | HD 136118 b
HD 136118 b is a brown dwarf located approximately 171 light-years away in the constellation of Serpens Cauda. This object had a minimum mass of 11.9 times that of Jupiter. Due to its high mass the planet is likely to be very hot and possibly glowing faintly. The lower limit on its mass is only slightly les... | 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... | 11,611 | zeroshot-train |
HD 14412 [SEP] constellation | HD 14412
HD 14412 (22 G. Fornacis) is the Henry Draper catalogue designation for an ordinary star in the southern constellation Fornax. It has an apparent visual magnitude of 6.33, which, according to the Bortle scale, can be dimly seen with the naked eye from rural locations. Based upon an annual parallax shift of 0.0... | Based upon models, it has 82% of the Sun's mass and 77% of the radius. HD 14412 is spinning with a projected rotational velocity of 3.26 km/s and is about 9.61 billion years old. The stellar atmosphere has an effective temperature of 5,359 K, giving it the yellow-hued glow of a G-type star.
HD 14412 has been examined f... | 11,612 | zeroshot-train |
HD 149382 [SEP] constellation | HD 149382
HD 149382 is a star in the constellation of Ophiuchus with an apparent visual magnitude of 8.943. This is too faint to be seen with the naked eye even under ideal conditions, although it can be viewed with a small telescope. Based upon parallax measurements, this star is located at a distance of about from th... | -alpha process). The effective temperature of the star's outer envelope is about 35,500 K, giving it the characteristic blue-white hue of a B-type star. HD 149382 has a visual companion located at an angular separation of 1 arcsecond.
In 2009, a substellar companion, perhaps even a superjovian planet, was announced orb... | 11,613 | zeroshot-train |
HD 153053 [SEP] constellation | HD 153053
HD 153053 is double star in the southern constellation of Ara. The brighter component is an A-type main sequence star that may be evolving into a subgiant. It has a twelfth magnitude visual companion at an angular separation of 24.7″ along a position angle of 52°. Mostly likely the two are isolated stars that... | radius of 49 AU from the host star.
External links.
- HR 6297
- CCDM J17001-5436
- Image HD 153053 | 11,614 | zeroshot-train |
HD 153201 [SEP] constellation | HD 153201
HD 153201 is a Bp star in the southern constellation of Ara. It is chemically peculiar star that displays an anomalous abundance of the element silicon in its spectrum. This is a suspected variable star of the type known as Alpha² Canum Venaticorum. There is a magnitude 9.86 companion star at an angular separ... | 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-... | 11,615 | zeroshot-train |
HD 154857 b [SEP] constellation | HD 154857 b
HD 154857 b is an extrasolar planet approximately 224 light years away in the constellation of Ara. This is a gas giant mass that orbits the star in an eccentric orbit. This planet was detected by using Anglo-Australian Telescope (AAT) UCLE spectrometer.
External links.
- Simulation HD 154857 b
- news.bbc.c... | Mikko Tuomi
Mikko Tuomi is a Finnish astronomer from the University of Hertfordshire, most known for his contributions to the discovery of a number of exoplanets, among them the Proxima Centauri b which orbits the closest star to the Sun. Mikko Tuomi was the first to find indications of the existence of Proxima Centaur... | 11,616 | zeroshot-train |
HD 158614 [SEP] constellation | HD 158614
HD 158614 is a spectroscopic binary star system approximately 60 light-years away in the constellation of Ophiuchus.
This system is in the Zeta Herculis moving group, which is of low metallicity stars, 5 billion years old. Besides ζ Herculis, the group includes δ Trianguli, ζ Reticuli, 1 Hydrae, Gl 456, φ Pav... | estimated the group velocity at 74.5 km/s. In 1970, Richard Woolley refined the list to ten stars, including φ Pavonis and ζ/ζ Reticuli as members of this cluster.
The parallel motion of the stars in this group implies a common origin, and hence a similar age and composition. The membership of ζ Herculis and HD 158614 ... | 11,617 | zeroshot-train |
HD 175167 b [SEP] constellation | HD 175167 b
HD 175167 b is an extra-solar planet orbiting HD 175167, which is a G type star within the Pavo constellation around 219 light years away from the Earth. The planet was discovered by the Magellan Planet Search Program as the astronomical object fit the Keplerian orbital model. During the observations 13 dop... | HD 86226
HD 86226 is a G type yellowish white star found in the constellation of Hydra.
Due to the reactions it had when placed under a Doppler test, 13 Magellan Doppler Velocity observations were made of an object found near the star. The object had a Keplerian orbit, was declared an exoplanet and dubbed HD 86226 b.
S... | 11,618 | zeroshot-train |
HD 175541 [SEP] constellation | HD 175541
HD 175541 is an intermediate-mass subgiant star in the constellation Serpens. That means when this star was a main-sequence, it was an A-type star. It is an 8th magnitude star about 410 light years from Earth. Despite its distance of over 100 ly, It was given the number 736 in the Gliese Catalogue of Nearby S... | 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... | 11,619 | zeroshot-train |
HD 178233 [SEP] constellation | HD 178233
HD 178233 is a 6th magnitude star in the constellation Lyra, approximately 133 light years from Earth. It is a white giant star of the spectral type F0III, meaning it possesses a surface temperature of 6,000 to 7,500 kelvins. It is hotter, much bigger, and much brighter than our Sun. | Battery D was reinforced to its authorized wartime strength.
Detachments from Btry A formed Btry 80-X in December 1941; a second detachment helped form the 804th CA (HD) Btry (Sep). Btry F at Sand Is. was designated the 807th CA (HD) Btry (Sep), while a second detachment helped organize the 715th CA (HD) Btry (Sep) 10-... | 11,620 | zeroshot-train |
HD 178911 [SEP] constellation | HD 178911
HD 178911 is a triple star system in the constellation Lyra. The secondary star (designated as HD 178911 B) has an apparent magnitude of 6.74 and a spectral type of G1V, which is very similar to our Sun at a distance of 160 light years. The age of the star is slightly older and have significantly higher metal... | HD 178911 Bb
HD 178911 Bb is a planet discovered in 2001 by Zucker who used the radial velocity method. The minimum mass of this giant planet is 7.35 times that of Jupiter that orbits close to the star. The period of the planet is 71.5 days and the semi-amplitude is 346.9 m/s. | 11,621 | zeroshot-train |
HD 187123 c [SEP] constellation | HD 187123 c
HD 187123 c is an extrasolar planet located approximately 156 light-years away in the constellation of Cygnus, orbiting the star HD 187123. This planet was published in 2006. The radius of the planet's orbit is 4.80 AU, 113 times more distant from the star than first companion. This takes 10 years to orbit.... | at apastron, the distance is 6.00 AU. The planet's mass is nearly 2 times that of Jupiter, but is likely to be smaller in size than the inner planet.
See also.
- HD 187123 b | 11,622 | zeroshot-train |
HD 188385 [SEP] constellation | HD 188385
HD 188385 is a star in the equatorial constellation of Aquila.
External links.
- HR 7589
- Image HD 188385 | 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-... | 11,623 | zeroshot-train |
HD 201507 [SEP] constellation | HD 201507
HD 201507 is a F-type subgiant in Equuleus.
Galactic orbit.
HD 201507 has a galactic orbit with an orbital eccentricity of 13.8%. | 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-... | 11,624 | zeroshot-train |
HD 208487 b [SEP] constellation | HD 208487 b
HD 208487 b is an extrasolar planet located approximately 144 light-years away in the constellation of Grus, orbiting the star HD 208487. This planet has a minimum mass close to half that of Jupiter and is most probably a gas giant. The planet orbits the star in a close, eccentric orbit. One revolution take... | they are orbiting. It involves a Bayesian statistical analysis of the radial-velocity data, using a prior probability distribution over the space determined by one or more sets of Keplerian orbital parameters. This analysis may be implemented using the Markov chain Monte Carlo (MCMC) method.
The method has been applied... | 11,625 | zeroshot-train |
HD 213240 b [SEP] constellation | HD 213240 b
HD 213240 b is an extrasolar planet located approximately 133 light-years (41 parsecs) away in the constellation of Grus, orbiting the star HD 213240.
The origin of this known planet came from the country of Switzerland and the astronomer Santos. The date was on April 4, 2001 and the method was Doppler spec... | HD 212301 b
HD 212301 b is an extrasolar planet located approximately 172 light-years (53 parsecs) away in the constellation of Octans, orbiting the star HD 212301. It has an orbital period of 2.25 Earth days. The orbital distance is 0.0341 astronomical units or 5.10 gigameters.
On August 22, 2005, taking place in ESO ... | 11,626 | zeroshot-train |
HD 215456 [SEP] constellation | HD 215456
HD 215456 is a star in the constellation Grus. With an apparent magnitude of 6.63, it is actually a yellow sunlike star located around 124 light-years distant from Earth. It has two planets that are around 32 and 76 times as massive as the earth that have periods of just under 192 and 2226 days respectively. ... | Gruis is a yellow star of magnitude 6.0 located around 106 light-years away. It may be a main sequence star or be just beginning to depart from the sequence as it expands and cools. In 2002 the star was found to have a planetary companion. HD 215456, HD 213240 and WASP-95 are yellow sunlike stars discovered to have two... | 11,627 | zeroshot-train |
HD 220074 [SEP] constellation | HD 220074
HD 220074 is a M2III red giant star located in Cassiopeia.
It had been considered K1V but is now known as M2III due to radius and surface gravity.
Planetary system.
From September 2008 to June 2012, the team B.-C. Lee, I. Han, and M.-G. Park observed HD 220074 with "the high-resolution spectroscopy of the fib... | Very-high-mass stars develop into supergiants that follow an evolutionary track that takes them back and forth horizontally over the HR diagram, at the right end constituting red supergiants. These usually end their life as a type II supernova. The most massive stars can become Wolf–Rayet stars without becoming giants ... | 11,628 | zeroshot-train |
HD 221287 b [SEP] constellation | HD 221287 b
HD 221287 b is an exoplanet approximately 173 light years away in the constellation of Tucana. This planet has mass 3.12 M (992 M) and orbits in a habitable zone at 1.25 AUs (6.06 μpc) from the star, taking 1.25 years to orbit at 29.9 km/s around the star. Naef discovered this planet in early 2007 by using ... | 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... | 11,629 | zeroshot-train |
HD 27894 [SEP] constellation | HD 27894
HD 27894 is a 9th magnitude star located approximately 143 light years away in the constellation of Reticulum. It is an orange dwarf (spectral type K2V), a type dimmer and cooler than our Sun.
In 2005, the Geneva Extrasolar Planet Search Team announced some of the discoveries of an extrasolar planet orbiting t... | HD 27894 b
HD 27894 b is a gas giant with a mass at least two thirds that of Jupiter, or twice that of Saturn. The distance from the planet to the star is one third compared that of Mercury from our Sun, and it takes almost exactly 18 days to complete one roughly circular orbit. | 11,630 | zeroshot-train |
HD 290327 b [SEP] constellation | HD 290327 b
HD 290327 b (also known as HIP 25191 b) is an extrasolar planet which orbits the G-type subgiant star HD 290327, located approximately 180 light years away in the constellation Orion. This planet has at least five halves the mass of Jupiter and takes 6.7 years to orbit the star at a semimajor axis of 3.35 A... | 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... | 11,631 | zeroshot-train |
HD 48265 b [SEP] constellation | HD 48265 b
HD 48265 b is an extrasolar planet located approximately 293 light-years away in the constellation of Puppis, orbiting the 8th magnitude G-type main sequence star HD 48265. This planet has a minimum mass of 1.47 times that of Jupiter. Because the inclination is not known, the true mass is not known. This pla... | HD 145377 b
HD 145377 b is an extrasolar planet located approximately 180 light-years awayThis planet was discovered on October 26, 2008 by Moutou "et al." using the HARPS spectrograph on ESO's 3.6 meter telescope installed at La Silla Observatory in Atacama desert, Chile.
See also.
- BD-17°63 b
- HD 131664
- HD 143361... | 11,632 | zeroshot-train |
HD 60532 [SEP] constellation | HD 60532
HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as our Sun (2.7 Gyr) and has me... | or Saturn-like planets. The star also hosts an asteroid belt at the region between middle planet to outer planet.
- On June 21, 2007, the first extrasolar planet found in the open cluster NGC 2423, was discovered around the red giant star NGC 2423-3. The planet is at least 10.6 times the mass of Jupiter and orbits at 2... | 11,633 | zeroshot-train |
HD 65216 [SEP] constellation | HD 65216
HD 65216 is an 8th magnitude G-type main sequence star located approximately away in the constellation of Carina. It is a Sun-like yellow dwarf, 8% less massive and somewhat less luminous. It cannot be seen without technical aid, but with binoculars or telescope it should be visible.
Planetary system.
An extra... | HD 216770
HD 216770 is an 8th magnitude star located approximately 124 light-years away in the constellation of Piscis Austrinus. It is an orange dwarf (spectral type K1 V), and is somewhat dimmer and cooler than our Sun.
In 2003 a planet was announced orbiting it by the Geneva Extrasolar Planet Search Team.
See also.
... | 11,634 | zeroshot-train |
HD 73256 [SEP] constellation | HD 73256
HD 73256, also known as CS Pyxidis, is a star located approximately 123 light years away in the constellation Pyxis. The spectral type is G8/K0V with a radius 0.94 times, luminosity 0.74 times and a mass 1.01 times that of the Sun. It is thought to be about a billion years old.
See also.
- HD 72659
- List of e... | HD 72659
HD 72659 is a yellow dwarf star in the Hydra constellation. The apparent magnitude is +7.48 and the distance is 168 light years away from Earth. An extrasolar planet was discovered orbiting this star in 2003.
See also.
- HD 73256
- List of extrasolar planets | 11,635 | zeroshot-train |
HD 73389 [SEP] constellation | HD 73389
HD 73389, also known as e² Carinae (e² Car), is a star in the constellation Carina. It is approximately 230 light years from Earth. It is an orange K-type giant with an apparent magnitude of +4.84. | 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-... | 11,636 | zeroshot-train |
HD 73534 [SEP] constellation | HD 73534
HD 73534 is an 8th magnitude G-type subgiant star located approximately 272 light years away in the constellation Cancer. A G5 star, it has evolved off the main sequence, which is why it is much more luminous than our Sun. In August 2009, it was announced that it has a planet. It is the first planetary system ... | HD 179079
HD 179079 is a G-type subgiant star in the constellation of Aquila. It has an apparent visual magnitude of approximately 7.96. It is larger than our Sun as it has a radius of approximately 1.48 solar radii. An exoplanet, HD 179079 b, was announced in August 2009 to be orbiting this star. The planet was detect... | 11,637 | zeroshot-train |
HD 93205 [SEP] constellation | HD 93205
HD 93205, or V560 Carinae, is a binary stellar system, in the Carina Nebula (NGC 3372) in the constellation Carina. It consists of two massive O-stars that revolve around each other in 6 days.
The more massive member of the pair is an O3.5 main sequence star. The spectrum shows some ionised nitrogen and helium... | 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-... | 11,638 | zeroshot-train |
HD 94510 [SEP] constellation | HD 94510
HD 94510 (u Car, u Carinae) is a star in the constellation Carina. It is an orange K-type giant with an apparent magnitude of +3.79 and is approximately 96.8 light years from Earth. It has about 22.3 times the sun's luminosity. | 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-... | 11,639 | zeroshot-train |
HD 96919 [SEP] constellation | HD 96919
HD 96919, also known by its Bayer designation of z Carinae and the variable star designation of V371 Carinae, is a blue supergiant star in the constellation Carina. It lies near the Carina Nebula and at a comparable distance.
V371 Car is an α Cyg variable, erratically pulsating and changing brightness by a few... | that are thought to indicate localised regions of enhanced mass loss.
HD 96919 is a B9 supergiant, possibly located 6,000 light years from Earth. It is considered to be a post red supergiant star, either evolving towards a Wolf-Rayet star or on a blue loop before returning to a cooler temperature. | 11,640 | zeroshot-train |
HIP 14810 c [SEP] constellation | HIP 14810 c
HIP 14810 c is an extrasolar planet approximately 165 light-years away in the constellation of Aries. This planet has mass at least 1.28 times that of Jupiter and orbits at 0.545 AU in an eccentric orbit. The planet was discovered by the N2K Consortium in 2006 and announced in a paper published in 2007. Wit... | planets c and d to likely be in a 2:1 resonance.
See also.
- Upsilon Andromedae
- HIP 14810
External links.
- Extrasolar Planet Interactions by Rory Barnes & Richard Greenberg, Lunar and Planetary Lab, University of Arizona | 11,641 | zeroshot-train |
HR 4072 [SEP] constellation | HR 4072
HR 4072 (ET Ursae Majoris, HD 89822, HIP 50933) is a star in the constellation Ursa Major. Its apparent magnitude is 4.94. Located around away, it is an α Canum Venaticorum variable of spectral type A1. | NGC 4072
NGC 4072 is a lenticular galaxy located 300 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Ralph Copeland on April 3, 1872 and is a member of the NGC 4065 Group.
NGC 4072 is classified as a LINER galaxy.
See also.
- List of NGC objects (4001–5000) | 11,642 | zeroshot-train |
HR 8799 b [SEP] constellation | HR 8799 b
HR 8799 b is an extrasolar planet located approximately 129 light-years away in the constellation of Pegasus, orbiting the 6th magnitude Lambda Boötis star HR 8799. It has a mass between 4 and 7 Jupiter masses and a radius from 10 to 30% larger than Jupiter's. It orbits at 68 AU from HR 8799 (or 7 AU inside t... | HR 8799 system. Along with two other planets orbiting HR 8799, the planet was discovered on November 13, 2008 by Marois "et al.", using the Keck and Gemini observatories in Hawaii. These planets were discovered using the direct imaging technique.
In 2009 it was discovered that the Hubble Space Telescope had in fact dir... | 11,643 | zeroshot-train |
IC 5146 [SEP] constellation | IC 5146
IC 5146 (also Caldwell 19, Sh 2-125, and the Cocoon Nebula) is a reflection/emission nebula and Caldwell object in the constellation Cygnus. The NGC description refers to IC 5146 as a cluster of 9.5 mag stars involved in a bright and dark nebula. The cluster is also known as Collinder 470. It shines at magnitud... | the bright open cluster M39. The cluster is about 4,000 ly away, and the central star that lights it formed about 100,000 years ago; the nebula is about 12 arcmins across, which is equivalent to a span of 15 light years.
When viewing IC 5146, dark nebula Barnard 168 (B168) is an inseparable part of the experience, for... | 11,644 | zeroshot-train |
Kappa Trianguli Australis [SEP] constellation | Kappa Trianguli Australis
Kappa Trianguli Australis (κ Trianguli Australis) is a star in the constellation Triangulum Australe.
Kappa Trianguli Australis is a yellow G-type supergiant with an apparent magnitude of +5.08. It is around 1,200 light years from Earth.
It is not generally listed as a variable star but Hippar... | system is an optical double. HD 147018 is a Sun-like star of apparent magnitude 8.3 and spectral type G9V, which was found to have two exoplanets, HD 147018 b and HD 147018 c, in 2009.
Of apparent magnitude 5.11, the yellow bright giant Kappa Trianguli Australis of spectral type G5IIa lies around distant from the Solar... | 11,645 | zeroshot-train |
Kepler-24 [SEP] constellation | Kepler-24
Kepler-24 is a star in the northern constellation of Lyra. It is located at the celestial coordinates: Right Ascension , Declination . With an apparent visual magnitude of 15.5, this star is too faint to be seen with the naked eye. | Kepler-61
Kepler-61 is a K-type main-sequence star approximately 1,100 light years from Earth in the constellation Cygnus. It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission used to detect planets that may be transiting their stars. On April 24, 2013 it was annou... | 11,646 | zeroshot-train |
Koposov II [SEP] constellation | Koposov II
Koposov II is a low-luminosity globular cluster in the constellation Gemini in the halo of the Milky Way galaxy. It was discovered, along with globular cluster Koposov I by S. Koposov et al. in 2007. Koposov I and Koposov II were described by their discoverers as the "lowest luminosity globular clusters orbi... | Koposov I
Koposov I is a low-luminosity globular cluster in the constellation Virgo in the halo of the Milky Way galaxy. It was discovered, along with globular cluster Koposov II by S. Koposov et al. in 2007. Koposov I and Koposov II were described by their discoverers as the "lowest luminosity globular clusters orbiti... | 11,647 | zeroshot-train |
MACHO-98-BLG-35 [SEP] constellation | MACHO-98-BLG-35
MACHO-98-BLG-35 was a gravitational microlensing event that occurred in July 1998 in the constellation Sagittarius. The red dwarf star causing the lens may have a planet, according to one study. | - M33 X-7 (most massive stellar-mass black hole known, not counting GW black holes)
- MACHO-96-BLG-5
- MACHO-96-NLG-5
- MACHO-98-BLG-6
- MACHO-99-BLG-22
- SN 1997D (in NGC 1536)
- SS 433
- V404 Cyg
- XTE J1118+480/KV UMa
- XTE J1550-564/V381 Nor
- XTE J1650-500 (at one time considered the smallest black hole known)
- X... | 11,648 | zeroshot-train |
Messier 89 [SEP] constellation | Messier 89
Messier 89 (M89 for short, also known as NGC 4552) is an elliptical galaxy in the constellation Virgo. It was discovered by Charles Messier on March 18, 1781. M89 is a member of the Virgo Cluster of galaxies.
Features.
Current observations indicate that M89 may be nearly perfectly spherical in shape. This is... | ) 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 ... | 11,649 | zeroshot-train |
NGC 1032 [SEP] constellation | NGC 1032
NGC 1032 is a spiral galaxy that is about 117 million light-years away in the constellation Cetus.
In January 2005 SN 2005E, a calcium-rich supernova, was discovered in NGC 1032. | SN 2005E
SN 2005E (aka 2005-1032) was a calcium-rich supernova first observed in January 2005 that scientists concluded was a new type of cosmic explosion. The explosion originated in the galaxy NGC 1032, approximately 100 million light years away.
brLocation: RA 02° 39' 14.34" Dec+01hr 05' 55.0" [Epoch J2000]
Researc... | 11,650 | zeroshot-train |
NGC 151 [SEP] constellation | NGC 151
NGC 151 is a mid-sized spiral galaxy located in the Cetus constellation.
The galaxy was discovered by English astronomer William Herschel on November 28, 1785. In 1886, Lewis Swift observed the same galaxy and catalogued it as NGC 153 and later was identified to be NGC 151.
The galaxy, viewed from almost face o... | , but 67 is not one more than a multiple of 18.
- palindromic in the consecutive bases 5 (232) and 6 (151).
In science.
- The atomic number of holmium, a lanthanide.
In science Astronomy.
- Messier object M67, a magnitude 7.5 open cluster in the constellation Cancer.
- The New General Catalogue object NGC 67, an ellipt... | 11,651 | zeroshot-train |
NGC 1579 [SEP] constellation | NGC 1579
NGC 1579 (also known as the Northern Trifid) is a diffuse nebula located in the constellation of Perseus. It is referred to as the Northern Trifid because of its similar appearance to the Trifid Nebula, which is located in the southern celestial hemisphere of the sky. It is a H II region, a region of star form... | 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... | 11,652 | zeroshot-train |
NGC 1868 [SEP] constellation | NGC 1868
NGC 1868 is a globular cluster in the Large Magellanic Cloud in the constellation Dorado. It was discovered by John Herschel in 1834.
External links.
- SIMBAD
- NASA/IPAC
- Flower, P. J., Geisler, D., Olszewski, E. W., & Hodge, P "NGC 1868 - A metal-poor intermediate-age cluster in the Large Magellanic Cloud"... | NGC 1398
NGC 1398 is an isolated barred spiral galaxy exhibiting a double ring structure. It is located 65 million light years from the Earth, in the constellation of Fornax. The galaxy, with a diameter of 135,000 light years, is slightly larger than the Milky Way. Over 100 billion stars are in the galaxy. It was first... | 11,653 | zeroshot-train |
NGC 19 [SEP] constellation | NGC 19
NGC 19 is a spiral galaxy in the Andromeda constellation. It was discovered by Lewis Swift on the 20th September 1885. It is often incorrectly listed as a duplicate of NGC 21.
NGC 19 in infared | NGC 203
NGC 203 is a lenticular galaxy located approximately 233 million light-years from the Solar System in the constellation Pisces. It was discovered on December 19, 1873 by Ralph Copeland.
The galaxy is also listed as NGC 211 in the New General Catalogue.
See also.
- Lenticular galaxy
- List of NGC objects (1–1000... | 11,654 | zeroshot-train |
NGC 20 [SEP] constellation | NGC 20
NGC 20 is a lenticular galaxy located in the Andromeda constellation. It was discovered on 18 September 1857 by R. J. Mitchell. The observation by Lewis Swift in 1885 led to the duplicate listing of the galaxy as NGC 6. | NGC 171
NGC 171 is a barred spiral galaxy with an apparent magnitude of 12, located around 3 million light-years away in the constellation Cetus. The galaxy has 2 main medium-wound arms, with a few minor arms, and a fairly bright nucleus and bulge. It was discovered on 20 October 1784 by William Herschel. It is also kn... | 11,655 | zeroshot-train |
NGC 2736 [SEP] constellation | NGC 2736
NGC 2736 (also known as the Pencil Nebula) is a small part of the Vela Supernova Remnant, located near the Vela Pulsar in the constellation Vela. The nebula's linear appearance triggered its popular name. It resides about 815 light-years (250 parsecs) away from the Solar System. It is thought to be formed from... | nebula is the brightest patch of a huge supernova remnant (Gum Nebula) whose delicate whisps cover the field. A relatively bright star is immersed in N2736 (mentioned by Herschel).
External links.
- Space.com article about NGC 2736
- NASA feature | 11,656 | zeroshot-train |
NGC 3504 [SEP] constellation | NGC 3504
NGC 3504 is a barred spiral galaxy in the constellation Leo Minor.
There is a large amount of molecular gas centered on the galactic nuculeus. Compared with other barred spiral galaxies, NGC 3504 is in an early phase of its evolution.
The mass of NGC 3504 has been difficult to narrow down, but it is believed t... | is estimated to be between based on kinematics of the water maser circumnuclear disk. The disk appears warped.
Nearby galaxies.
NGC 2273 is the brightest galaxy in a galaxy group known as the NGC 2273 group. Other members of the group include the galaxies NGC 2237B and UGC 3504. NGC 2237B lies 40 arcminutes to the sout... | 11,657 | zeroshot-train |
NGC 428 [SEP] constellation | NGC 428
NGC 428 is a barred spiral galaxy in the constellation of Cetus (The Sea Monster), with its spiral structure distorted and warped, possibly the result of the collision of two galaxies. There appears to be a substantial amount of star formation occurring within NGC 428 and lacks well defined arms — a telltale si... | NGC 428 has been compared to NGC 5645.
Discoveries.
NGC 428 was discovered by William Herschel in December 1786. A type Ia supernova designated "SN2013ct" was discovered May 11, 2013, within the galaxy by Stuart Parker of the Backyard Observatory Supernova Search (BOSS) project in Australia and New Zealand.
Smoker et a... | 11,658 | zeroshot-train |
NGC 4308 [SEP] constellation | NGC 4308
NGC 4308 is an elliptical galaxy in the constellation Coma Berenices. It is a member of the Coma I Group. | the Nearby Optical Galaxy sample of Giuricin et al.
Other possible member galaxies (galaxies listed in only one or two of the lists from the above references) include IC 3215, IC 3247, MCG 5-29- 66, NGC 4080, NGC 4150, NGC 4308, NGC 4455, NGC 4509, NGC 4534, NGC 4627, NGC 4631, NGC 4656, NGC 4670, UGC 6900, UGC 7007, U... | 11,659 | zeroshot-train |
NGC 4444 [SEP] constellation | NGC 4444
NGC 4444 is an intermediate spiral galaxy in the constellation Centaurus. The morphological classification places it midway on the continuum between a barred spiral (SB) and an unbarred spiral (SA), with an inner region that lies between a ring-like ("r") and a purely spiral form ("s"), and medium- ("b") to lo... | 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... | 11,660 | zeroshot-train |
NGC 4517 [SEP] constellation | NGC 4517
NGC 4517 is a spiral galaxy located approximately 40 million light-years away in the constellation of Virgo. It was discovered in 1784 by William Herschel. | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,661 | zeroshot-train |
NGC 6086 [SEP] constellation | NGC 6086
NGC 6086 is an elliptical galaxy in the constellation of Corona Borealis. It has an apparent magnitude of 12.7. A Type-cD galaxy, it is the brightest cluster galaxy in the cluster Abell 2162. In 2010, a supermassive black hole was discovered in NGC 6086. | the brightest within Caldwell Objects in the constellation Coma Berenices
- NGC 6086
- QSO 0957, the first identified gravitationally lensed object
- 3C 401
See also.
- Giant elliptical galaxy (gE)
- Giant galaxy
- Elliptical galaxy (E#)
- Lenticular galaxy (S0, SA0, SAB0, SB0, E9)
- Type-D galaxy
Further reading.
- PD... | 11,662 | zeroshot-train |
NGC 6144 [SEP] constellation | NGC 6144
NGC 6144 is a globular cluster in the constellation Scorpius.
External links.
- Globular Clusters Database | NGC 48
The New General Catalogue object NGC 48 is a barred spiral galaxy located approximately 79.3 million light-years from the Solar System in the constellation Andromeda.
See also.
- Spiral galaxy
- List of NGC objects (1–1000)
- Andromeda (constellation)
External links.
- http://spider.seds.org/ngc/ngc.cgi?48
- htt... | 11,663 | zeroshot-train |
NGC 6356 [SEP] constellation | NGC 6356
NGC 6356 is a globular cluster located in the constellation Ophiuchus. It is designated as II in the galaxy morphological classification scheme and was discovered by the German-born British astronomer William Herschel on 18 June 1784. The star cluster is more dense and bright towards the middle. 6356 is locate... | to the northeast of M9 is the dimmer globular cluster NGC 6356, while at about 80' to the southeast is the globular NGC 6342.
External links.
- Messier 9, SEDS Messier pages
- M9, Galactic Globular Clusters Database page
- The glittering stars of Messier 9, March 16, 2012, Tg Daily Staff, "TG Daily" | 11,664 | zeroshot-train |
OGLE-2005-BLG-169Lb [SEP] constellation | OGLE-2005-BLG-169Lb
OGLE-2005-BLG-169Lb is an extrasolar planet located approximately 2700 parsecs away in the constellation of Sagittarius, orbiting the star OGLE-2005-BLG-169L. This planet was discovered by the OGLE project using the gravitational microlensing method. Based on a most likely mass for the host star of ... | OGLE-2007-BLG-368Lb
OGLE-2007-BLG-368Lb is an extrasolar planet located approximately 19,230 light-years away in the constellation of Scorpius, orbiting the star OGLE-2007-BLG-368L. This planet was detected on December 8, 2009 by the gravitational microlensing by Sumi. It has mass 6.94% of Jupiter (i.e. 22 times that o... | 11,665 | zeroshot-train |
PV Telescopii [SEP] constellation | PV Telescopii
PV Telescopii (also known as HD 168476) is a class B-type (blue) supergiant extreme helium star in the constellation Telescopium. It is also the prototype of variable stars called PV Telescopii variables.
Properties.
PV Telescopii shows radial velocity changes thought to be due to radial pulsations caused... | BX Circini
BX Circini is a star in the constellation Circinus. Its variability was discovered in 1995, with its apparent magnitude ranging from 12.57 to 12.62 over a period of 2 hours 33 minutes. It is currently classified as a PV Telescopii variable star, but has been put forward as the prototype of a new class of pul... | 11,666 | zeroshot-train |
RX J1856.5-3754 [SEP] constellation | RX J1856.5−3754
RX J1856.5−3754 (also called RX J185635−3754, RX J185635−375, and various other designations) is a nearby neutron star in the constellation Corona Australis.
Discovery and location.
RX J1856.5−3754 is thought to have formed in a supernova explosion of its companion star about one million years ago and i... | 400 km/s) to the newly formed neutron star.
Some of the closest known neutron stars are RX J1856.5−3754, which is about 400 light-years from Earth, and PSR J0108−1431 at about 424 light years. RX J1856.5-3754 is a member of a close group of neutron stars called The Magnificent Seven. Another nearby neutron star that wa... | 11,667 | zeroshot-train |
Red Square Nebula [SEP] constellation | Red Square Nebula
The Red Square Nebula is a celestial object located in the area of the sky occupied by star MWC 922 in the constellation Serpens. The first images of this bipolar nebula, taken using the Mt. Palomar Hale telescope in California, were released in April 2007. It is notable for its square shape, which ac... | March 2013.
Features Deep-sky objects.
Of the deep-sky objects of interest in Vela is a planetary nebula known as the NGC 3132, nicknamed the 'Eight-Burst Nebula' or 'Southern Ring Nebula' (see accompanying photo). It lies on the border of the constellation with Antlia. NGC 2899 is an unusual red-hued example. This con... | 11,668 | zeroshot-train |
Simeis 147 [SEP] constellation | Simeis 147
Simeis 147, also known as the Spaghetti Nebula, SNR G180.0-01.7 or Sharpless 2-240, is a supernova remnant (SNR) in the Milky Way, straddling the border between the constellations Auriga and Taurus. Discovered in 1952 at the Crimean Astrophysical Observatory using a 25-inch Schmidt-Cassegrain telescope, it i... | WestPac/Vietnam aboard in 1970, and in 1971-72. From April 1972 in response to the Easter Offensive, the squadron participated in Operation Freedom Train, tactical air sorties against military and logistic targets in South Vietnam and the southern part of North Vietnam. In March–June 1973 embarked on "Constellation", V... | 11,669 | zeroshot-train |
Swift J1745-26 [SEP] constellation | Swift J1745-26
Swift J1745-26 is a stellar-mass black hole located a few degrees from the center of the Milky Way galaxy toward the constellation Sagittarius. It was discovered by NASA's Swift satellite on September 16, 2012 due to the detection of an X-ray nova. The pattern of X-rays from the nova indicated that the c... | resides about 20,000 to 30,000 light-years away in the galaxy's inner region. Ground-based observatories have detected infrared and radio emissions from Swift J1745-26, but thick clouds of obscuring dust have prevented astronomers from catching Swift J1745-26 in visible light.
Swift J1745-26 must be a member of a low-m... | 11,670 | zeroshot-train |
Tau Ophiuchi [SEP] constellation | Tau Ophiuchi
Tau Ophiuchi (τ Oph) is a multiple star in the constellation Ophiuchus, approximately 167 light years away based on parallax. Its two main components are two yellow-white main sequence stars, A, of magnitude 5.24 and class F2V, and B, of magnitude 5.94 and class F5V, orbiting each other with a period of 25... | part of (), meaning "Left Wall of Heavenly Market Enclosure." The stars in this group include ν Ophiuchi, δ Herculis, λ Herculis, μ Herculis, ο Herculis, 112 Herculis, ζ Aquilae, θ Serpentis, η Serpentis, ξ Serpentis and η Ophiuchi. Consequently, ν Ophiuchi itself is known as (, ), and together with ζ Capricorni repres... | 11,671 | zeroshot-train |
UX Arietis [SEP] constellation | UX Arietis
UX Arietis is a triple star system located in the northern zodiacal constellation of Aries. Based upon parallax measurements from the Hipparcos satellite, it is roughly 168 light years away. The primary, component Aa, is a variable star of the RS CVn type. The variability of the star is believed due to a com... | up 3.5%, compared to the 81% of men's coverage. The lengths of these articles were 25–27% shorter than the length of men's articles. There was an international frenzy in 2012 when the first woman that represented Saudi Arabia in the 2012 Olympics competed in track. That was the most women's sports coverage that there h... | 11,672 | zeroshot-train |
W33A [SEP] constellation | W33A
W33A is a protostar located approximately 12,000 light-years away from Earth, in the constellation Sagittarius. As a star in the early stages of formation, so has attracted the interest of astronomers, who observed that while the protostar is accumulating material from surrounding clouds of gas and dust, it is sim... | ; Schutte, W. A.; Boogert, A. C. A.; Chiar, J. E.; Ehrenfreund, P.; Gerakines, P. A.; Keane, J. V.; Tielens, A. G. G. M.; van Dishoeck, E. F.; and Kerkhof, O., The Astrophysical Journal, Volume 536, Issue 1, pp. 347–356, DOI: 10.1086/308940, Harvard University
- VLTI/MIDI 10 μm Interferometry of the Forming Massive Sta... | 11,673 | zeroshot-train |
Wolf 1061 [SEP] constellation | Wolf 1061
Wolf 1061 (also known as HIP 80824 and V2306 Ophiuchi) is an M class red dwarf star located about 14.1 light years away in the constellation Ophiuchus. It is the 36th closest known star system to the Sun and has a relatively high proper motion of 1.2 seconds of arc per year. Like many red dwarfs, it most like... | Gliese 876
Gliese 876 is a red dwarf approximately 15 light-years away from Earth in the constellation of Aquarius. It is the one of the closest known stars to the Sun confirmed to possess a planetary system and the fifth closest such system known to consist of multiple planets (after Wolf 1061, Kapteyn's Star, Tau Cet... | 11,674 | zeroshot-train |
Xi Sagittarii [SEP] constellation | Xi Sagittarii
The Bayer designation Xi Sagittarii (ξ Sagittarii) is shared by two stars, ξ Sagittarii and ξ² Sagittarii, in the constellation Sagittarius, separated by 0.46° in the sky. Because they are close to the ecliptic, they can be occulted by the Moon and, very rarely, by planets. The last occultation of ξ² Sagi... | Comencho Lake
Comencho Lake is a body of water in the Broadback River watershed in the Eeyou Istchee James Bay (municipality) area within the Nord-du-Québec, in the province of Quebec, in Canada. This lake is part of the territory of the Assinica Wildlife Sanctuary.
Forestry is the main economic activity of the sector.... | 11,675 | zeroshot-train |
Zeta Herculis [SEP] constellation | Zeta Herculis
Zeta Herculis (ζ Her, ζ Herculis) is a multiple star system in the constellation Hercules. It has a combined apparent visual magnitude of 2.81, which is readily visible to the naked eye. Parallax measurements put it at a distance of about from Earth.
The primary member is a subgiant star that is somewhat ... | HD 158614
HD 158614 is a spectroscopic binary star system approximately 60 light-years away in the constellation of Ophiuchus.
This system is in the Zeta Herculis moving group, which is of low metallicity stars, 5 billion years old. Besides ζ Herculis, the group includes δ Trianguli, ζ Reticuli, 1 Hydrae, Gl 456, φ Pav... | 11,676 | zeroshot-train |
16 Aquarii [SEP] constellation | 16 Aquarii
16 Aquarii, abbreviated 16 Aqr, is a star in the constellation of Aquarius. "16 Aquarii" is the Flamsteed designation. It is a faint star, just visible to the naked eye, with an apparent visual magnitude of 5.869. Based upon an annual parallax shift of , it is located about 342 light years away. It is moving... | 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... | 11,677 | zeroshot-train |
28 Monocerotis [SEP] constellation | 28 Monocerotis
28 Monocerotis is a class K4III (orange giant) star in the constellation Monoceros. Its apparent magnitude is 4.69 and it is approximately 450 light years away based on parallax.
It is an FK Comae Berenices variable, with a magnitude varying by 0.02 with a period of 0.21 days. | Laurie Sawle
Lawrence Michael "Laurie" Sawle (born 19 August 1925 at East Fremantle, Western Australia) is a former first-class cricketer and chairman of selectors for the Australian national team.
Laurie Sawle served in the 7th Australian Infantry Battalion during the Second World War. He enlisted in January 1944 and ... | 11,678 | zeroshot-train |
7 Arietis [SEP] constellation | 7 Arietis
7 Arietis (abbreviated 7 Ari) is a binary star system in the northern constellation of Aries. "7 Arietis" is the Flamsteed designation. The pair have a combined apparent visual magnitude of 5.76, making it faintly visible to the naked eye from dark suburban skies. Based upon an annual parallax shift of 5.85 m... | MV Mefküre
MV "Mefküre (often referred to as Mefkura") was a Turkish wooden-hulled motor schooner chartered to carry Jewish Holocaust refugees from Romania to Istanbul, sailing under the Turkish and Red Cross flags. On 5 August 1944 a Soviet submarine sank her in the Black Sea by shellfire, killing more than 300 refuge... | 11,679 | zeroshot-train |
7 Cancri [SEP] constellation | 7 Cancri
7 Cancri (7 Cnc) is a giant star in the constellation Cancer. Its apparent magnitude is 6.84 and it is about away.
The annual parallax of 7 Cancri determined from the Hipparcos satellite mission is , giving a distance of with an 11.5% margin of error. The more recent and more accurate Gaia Data Release 2 conta... | Côte-d'Or's 4th constituency
The 4th constituency of the Côte-d'Or is a French legislative constituency in the Côte-d'Or "département".
Description.
Côte-d'Or's 4th constituency is a large rural seat covering the north of the department. Historically it has supported the non-Gaullist conservative Union for French Democ... | 11,680 | zeroshot-train |
90 Tauri [SEP] constellation | 90 Tauri
90 Tauri (90 Tau) is a star in the zodiac constellation of Taurus, located 144 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.27. 90 Tauri is a member of the Hyades cluster and is listed as a double star.
This is an A-type main-s... | was captured on video, footage of which later becomes the single "Speed Up".[7]
“Speed Up” quickly zooms to the top of the Kamenitza Rock 40 chart on Z-Rock Radio and maintains a position in its top 10 for 30 weeks.[23] During 2013, Sevi does a lot of performances on motorcycle meetings and festivals, including perform... | 11,681 | zeroshot-train |
A Centauri [SEP] constellation | A Centauri
A Centauri (A Cen) is a star in the constellation Centaurus. It is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.62 and is approximately 430 light years from Earth.
External links.
- Wikisky image of HD 100673 (A Centauri) | Sykes, 6th Baronet
- Robert Syms
List of MPs T.
- John Ellis Talbot
- Thomas Tapling
- Sir Peter Taspsell; MP for Horncastle (1966–1983), East Lindsey (1983–1997) and Louth and Horncastle (1997–2015)
- Mavis Tate
- Charles Taylor (UK politician)
- Edwin Taylor (British politician)
- Frank Taylor (UK politician)
- Hugh ... | 11,682 | zeroshot-train |
AB Doradus [SEP] constellation | AB Doradus
AB Doradus is a pre-main-sequence quadruple star system in the constellation Dorado. The primary is a flare star that shows periodic increases in activity.
The primary star in this system spins at a rate 50 times that of the Sun, and consequently has a strong magnetic field. It has a greater number of star s... | semi-major axis. It is a gas giant located in the constellation of Pisces, 155 light-years from the Solar System, and estimated to have a mass nine to thirteen times that of Jupiter, and a surface temperature of 1000 K.
It is a relatively young stellar system, part of the AB Doradus moving group of ca. 30 main stars cr... | 11,683 | zeroshot-train |
Alpha Circini [SEP] constellation | Alpha Circini
Alpha Circini (α Cir, α Circini) is a variable star in the faint, southern, circumpolar constellation of Circinus. At an apparent visual magnitude of 3.19, it is the brightest star in the constellation and can be readily seen with the naked eye from the southern hemisphere. Parallax measurements of this s... | voted in favour of it. He stood as a pro-Treaty Sinn Féin candidate at the 1922 general election but was not elected.
Following the formation of the Irish Free State he became County Meath's first State Solicitor, a role which involves being the top appellate advocate, amongst other duties.
After public life he continu... | 11,684 | zeroshot-train |
Alpha Telescopii [SEP] constellation | Alpha Telescopii
Alpha Telescopii, Latinized from α Telescopii, is the brightest star in the southern constellation of Telescopium, with an apparent visual magnitude of 3.5. The ancient Roman astronomer Ptolemy included it in the constellation Corona Australis, but it was moved to Telescopium when that constellation wa... | and , while the declination coordinates are between −45.09° and −56.98°. The whole constellation is visible to observers south of latitude 33°N.
Features.
Features Stars.
Within the constellation's borders, there are 57 stars brighter than or equal to apparent magnitude 6.5. With a magnitude of 3.5, Alpha Telescopii is... | 11,685 | zeroshot-train |
Arches Cluster [SEP] constellation | Arches Cluster
The Arches Cluster is the densest known star cluster in the Milky Way located about 100 light-years from its center, in the constellation Sagittarius (The Archer), 25,000 light-years from Earth.
The discovery of this cluster was reported by Nagata et al. in 1995, and independently by Cotera et al. in 199... | Fornax Cluster
The Fornax Cluster is a cluster of galaxies lying at a distance of 19 megaparsecs (62 million light-years). It is the second richest galaxy cluster within 100 million light-years, after the considerably larger Virgo Cluster, and may be associated with the nearby Eridanus Group. It lies primarily in the c... | 11,686 | zeroshot-train |
Delta Telescopii [SEP] constellation | Delta Telescopii
The Bayer designation Delta Telescopii (δ Tel, δ Telescopii) is shared by two stars in the southern constellation Telescopium. They are separated by 0.16° on the sky.
- δ Telescopii
- δ Telescopii | and is estimated to be 5.2±0.4 times as massive and have 3.3±0.5 times the Sun's radius. Close by Alpha Telescopii are the two blue-white stars sharing the designation of Delta Telescopii. Delta¹ Telescopii is of spectral type B6IV and apparent magnitude 4.9, while Delta² Telescopii is of spectral type B3III and magnit... | 11,687 | zeroshot-train |
Engraved Hourglass Nebula [SEP] constellation | Engraved Hourglass Nebula
The Engraved Hourglass Nebula (also known as MyCn 18) is a young planetary nebula in the southern constellation Musca. It was discovered by Annie Jump Cannon and Margaret W. Mayall during their work on an extended Henry Draper Catalogue (the catalogue was built between 1918 and 1924). At the t... | visual effects studio started by Dave McKean
- "Hourglass", a 1995 film directed by C. Thomas Howell
Books.
- "Hourglass" (Kiš novel), a Danilo Kiš
- "Hourglass" (Gray novel), a 2010 novel written by Claudia Gray
- "Hourglass", a 2004 episode from season 3 of "Alias"
- The Hourglass, a supervillain character from the 2... | 11,688 | zeroshot-train |
Epsilon Phoenicis [SEP] constellation | Epsilon Phoenicis
Epsilon Phoenicis is a star in the constellation Phoenix. Its apparent magnitude is 3.87. Located around distant, it is an orange giant of spectral type K0III, a star that has used up its core hydrogen and has expanded. | - "A Mother's Love" (2013)
- "The Beekeeper's Daughter" (2014)
- "Songs of Love and War" (2015) (The first of "The Deverill Chronicles")
- "Daughters of Castle Deverill" (2016) (The second of "The Deverill Chronicles")
- "Last Secret of the Deverills" (2017) (The third of "The Deverill Chronicles")
- "The Temptation of... | 11,689 | zeroshot-train |
Fleming 1 [SEP] constellation | Fleming 1
Fleming 1 is an unusual planetary nebula situated in the Centaurus constellation. It has a pair of symmetrical jets spanning more than 2.8 pc and delineated with a number of knots. The jets and knots are moving away from the center of the nebula and were probably ejected 10,000 to 16,000 year ago. The innermo... | Air Transport Wing, Heavy, 18 Jan 1963
- 437th Military Airlift Wing, 8 Jan 1966-1 October 1991
History Stations.
- Accra Airfield, British Gold Coast, 17 Aug 1942-30 Sep 1943
- Wheelus Air Base, Libya, 20 Jul 1952-12 Apr 1954
- Charleston AFB, South Carolina, 13 Apr 1954-1 October 1991
History Aircraft.
- C-54 Skymast... | 11,690 | zeroshot-train |
GJ 526 [SEP] constellation | GJ 526
GJ 526 (Lalande 25372, Wolf 498) is a red dwarf star in the northern constellation of Boötes. It has an apparent visual magnitude of 8.5, which is too faint to be seen with the naked eye. Based upon an annual parallax shift of 0.184 arc seconds as measured by the Hipparcos satellite, this system is from Earth.
H... | 1847 edition of Lalande's catalogue by Francis Baily it was assigned number 25372, since it sometimes designated as "Lalande 25372" or "LAL 25372".
High proper motion of this star and its large parallax were known at least from 1911, when Frank Schlesinger published a paper where he announced its parallax and mentioned... | 11,691 | zeroshot-train |
Gamma Delphini [SEP] constellation | Gamma Delphini
Gamma Delphini, Latinized from γ Delphini, is a binary star system approximately 101 light-years away in the constellation of Delphinus. The star marks one corner of the asterism "Job's Coffin". It is one of the best known double stars in the sky, consisting of a fourth magnitude orange subgiant and a fi... | September 2016 and it is now so included in the List of IAU-approved Star Names.
In Chinese, (), meaning "Good Gourd", refers to an asterism consisting of Alpha Delphini, Gamma Delphini, Delta Delphini, Beta Delphini and Zeta Delphini. Consequently, the Chinese name for Alpha Delphini itself is (, ).
In Hindu astronomy... | 11,692 | zeroshot-train |
Gamma Trianguli [SEP] constellation | Gamma Trianguli
Gamma Trianguli (Gamma Tri, γ Trianguli, γ Tri) is a star in the constellation Triangulum located approximately 112 light years from Earth. It has an apparent magnitude of +4.01 and forms an optical (line-of-sight) triple with Delta Trianguli and 7 Trianguli.
Properties.
This star has a stellar classifi... | stars their Bayer designations in 1756.
Alpha Trianguli Australis, known as Atria, is a second-magnitude orange giant and the brightest star in the constellation, as well as the 42nd-brightest star in the night sky. Completing the triangle are the two white main sequence stars Beta and Gamma Trianguli Australis. Althou... | 11,693 | zeroshot-train |
Gliese 667 [SEP] constellation | Gliese 667
Gliese 667 (142 G. Scorpii) is a triple-star system in the constellation Scorpius lying at a distance of about 6.8 pc (23.6 ly) from Earth. All three of the stars have masses smaller than the Sun. There is a 12th magnitude star close to the other three, but it is not gravitationally bound to the system. To t... | Gliese 667 Cb
Gliese 667 Cb is an exoplanet orbiting the star Gliese 667 C, a member of the Gliese 667 triple-star system. It is the most massive planet discovered in the system and is likely a super-Earth or a mini-Neptune. Orbital-stability analysis indicates that it cannot be more than twice its minimum mass. It orb... | 11,694 | zeroshot-train |
Gum Nebula [SEP] constellation | Gum Nebula
The Gum Nebula (Gum 12) is an emission nebula that extends across 36° in the southern constellations Vela and Puppis. It lies roughly 350 parsecs from the Earth. Hard to distinguish, it was widely believed to be the greatly expanded (and still expanding) remains of a supernova that took place about a million... | NGC 6334
NGC 6334 (also known as the Cat's Paw Nebula, Bear Claw Nebula, or Gum 64) is an emission nebula and star-forming region located in the constellation Scorpius. It was discovered by astronomer John Herschel in 1837, who observed it from the Cape of Good Hope in South Africa.
External links.
- On the Trail of a ... | 11,695 | zeroshot-train |
HD 110073 [SEP] constellation | HD 110073
HD 110073 (Bayer designation l Cen / l Centauri) is a star in the constellation Centaurus. It is a blue-white B-type bright giant with an apparent magnitude of +4.63 and is approximately 365 light years from Earth.
This is a single-lined spectroscopic binary star system that belongs to the Pleiades group. | 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-... | 11,696 | zeroshot-train |
HD 115337 [SEP] constellation | HD 115337
HD 115337 is a cool supergiant star in the constellation Camelopardalis. It has an apparent magnitude of 6.272 so it is visible under very dark conditions. It is about 680 light-years or 210 parsecs away. It has a much fainter A8 main sequence companion.
See also.
- Red supergiant | 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-... | 11,697 | zeroshot-train |
HD 128311 c [SEP] constellation | HD 128311 c
HD 128311 c is an exoplanet located approximately 54 light-years away in the constellation of Boötes. This planet orbits in an eccentric orbit at 1.76 AU from its star (HD 128311). The planet has minimum mass 3.22 Jupiter masses. | 128311 b is the smaller planet, with a mass of ; it was discovered through radial velocity observations. It orbits at almost the same distance as Earth, at 1.099 AU; however, its orbital period is significantly longer at 448.6 days.
The larger of the two, HD 128311 c, has a mass of and was discovered in the same manne... | 11,698 | zeroshot-train |
HD 142 [SEP] constellation | HD 142
HD 142 is a 6th magnitude yellow-white dwarf star approximately 85.5 light years away in the constellation of Phoenix. A companion star was detected in 1894 making this a binary star system. The binary companion was confirmed in 2007 and determined to be of spectral type K8.5-M1.5 with a mass 59% that of the sun... | 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... | 11,699 | zeroshot-train |
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