12B (disambiguation)

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12B is a 2001 Indian Tamil-language film by Jeeva.

12B may also refer to:

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Vitamin B12 is a water-soluble vitamin with a key role in the normal functioning of the brain and nervous system, and for the formation of blood.

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9D or 9-D can refer to:

<span class="mw-page-title-main">OGLE-TR-56b</span> Hot Jupiter orbiting OGLE-TR-56

OGLE-TR-56b is an extrasolar planet located approximately 1500 parsecs or 5000 light years 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 confirmed on January 4, 2003 by the Doppler technique. The period of this confirmed planet was the shortest until the confirmed discovery of WASP-12b on April 1, 2008. The short period and proximity of the OGLE-TR-56 b to its host mean it belongs to a class of objects known as hot Jupiters.

8B or VIII-B may refer to :

<span class="mw-page-title-main">New York State Route 12B</span> State highway in New York, US

New York State Route 12B (NY 12B) is a state highway in the central part of New York in the United States. NY 12B is a north–south highway connecting Oneida County in the north to Chenango County in the south, passing through Madison County in between. The southern terminus of NY 12B is at NY 12 in the village of Sherburne. The northern terminus is at NY 5 in the town of New Hartford. In Madison County, NY 12B directly abuts the campus of Colgate University in the village of Hamilton.

<span class="mw-page-title-main">HAT-P-3b</span> Jovian-sized exoplanet orbiting HAT-P-3

HAT-P-3b, also named Teberda, is an extrasolar planet that orbits the star HAT-P-3 approximately 450 light-years away in the constellation of Ursa Major. It was discovered by the HATNet Project via the transit method and confirmed with Doppler spectroscopy, so both its mass and radius are known quite precisely. Based on these figures it is predicted that the planet has about 75 Earth masses' worth of heavy elements in its core, making it similar to the planet HD 149026 b.

<span class="mw-page-title-main">WASP-12b</span> Hot Jupiter exoplanet in the constellation Auriga

WASP-12b is a hot Jupiter orbiting the star WASP-12, discovered in April of 2008, by the SuperWASP planetary transit survey. The planet takes only a little over one Earth day to orbit its star, in contrast to about 365.25 days for the Earth to orbit the Sun. Its distance from the star is only the Earth's distance from the Sun, with an eccentricity the same as Jupiter's. Consequently, it has one of the lowest densities for exoplanets. On December 3, 2013, scientists working with the Hubble Space Telescope (HST) reported detecting water in the atmosphere of the exoplanet. In July 2014, NASA announced finding very dry atmospheres on three exoplanets orbiting sun-like stars.

WASP-12 is a magnitude 11 yellow dwarf star located approximately 1347 light-years away in the constellation Auriga. WASP-12 has a mass and radius similar to the Sun and is known for being orbited by a planet that is extremely hot and has a retrograde orbit around WASP-12. WASP-12 forms a triple star system with two red dwarf companions. Both of them have spectral types of M3V and are only 38% and 37% as massive as the Sun, respectively.

7B or VII-B may refer to :

9B, 9b or IX-B may refer to :

5B or 5-B may refer to:

11B may refer to :

HAT-P-8 is a magnitude 10 star located 700 light-years away in Pegasus. It is a F-type star about 28% more massive than the Sun. Two red dwarf companions have been detected around HAT-P-8. The first has a spectral type of M5V and has a mass of 0.22 M. The second is even less massive, at 0.18 M, and its spectral type is M6V.

<span class="mw-page-title-main">HAT-P-12b</span> Extrasolar planet in constellation Canes Venatici

HAT-P-12b, formally named Puli, is an extrasolar planet approximately 468 light years away from Earth, orbiting the 13th magnitude K-type star HAT-P-12, which is located in Canes Venatici constellation. It is a transiting hot Jupiter that was discovered by the HATNet Project on April 29, 2009.

B21 may refer to:

PSR J1544+4937 is a pulsar and gamma-ray source. A millisecond pulsar, it has a very short rotation period of 2.16 milliseconds. It has a planet or brown dwarf, PSR J1544+4937 b.