astro.wikisort.org - Meteorite

51 Eridani b is a "Jupiter-like" planet that orbits the young F0 V star 51 Eridani, in the constellation Eridanus.[3] It is 96 light years away from the solar system, and it is approximately 20 million years old.[4]

51 Eri b

Direct imaging of 51 Eri b
Discovery
Discovered by	Macintosh et al.
Discovery date	Dec 2014
Detection method	Imaged
Orbital characteristics
Semi-major axis	11.1+4.2 −1.3 AU
Eccentricity	0.49 (± 0.15) [1]
Orbital period (sidereal)	10260+6300 −1800 d
Inclination	136.0 (± 11.0) [1] deg
Time of periastron	2452014.79 (± 12.0) [1] JD
Argument of periastron	84.0 (± 58.0) [1] deg
Star	51 Eridani
Physical characteristics
Mean radius	1.11+0.16 −0.13 RJ
Mass	2.6 (± 0.3) MJ
Surface gravity	3.5 g
Temperature	700 K[2]

Discovery

51 Eridani b was announced in August 2015, but was discovered in December 2014 using the Gemini Planet Imager, an international project led by the Kavli Institute for Particle Astrophysics and Cosmology. 51 Eridani b is the first exoplanet discovered by the Gemini Planet Imager.[5] The Gemini Planet Imager was specifically created to discern and evaluate dim, newer planets orbiting bright stars through “direct imaging.”[6] Direct imaging allows astronomers to use adaptive optics to sharpen the resolution of the image of a target star, then obstruct its starlight.[6] Any residual incoming light is then scrutinized, and the brightest spots suggest a possible planet.[6] Prior to the discovery of 51 Eridani b, each of the directly imaged worlds previously discovered had been gas giants many times the mass of Jupiter.[7]

Physical characteristics

The planet has a mass at least 2.6M_J, but not more than 11M_J.[8] Its radius is about 1.11 times the radius of Jupiter. It orbits 11.1 AU from its host star, and has an orbital period of roughly 10,000 days.[1] The average temperature is 700 K, which is substantially hotter than the 130 K average temperature of Jupiter, the planet in the Solar System of closest size.[9] It has the second strongest methane signature of any exoplanet, after GJ 504 b.[10] This methane signature, along with the low luminosity of the object, should produce additional clues as to how 51 Eridani b was formed.[5] Astronomers also detected the presence of water in the planet's spectrum.[11] Atmospheric modeling favors a low surface gravity and a partly cloudy atmosphere.[7]

References

На других языках

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[de] 51 Eridani b

51 Eridani b ist ein Exoplanet, der den rund 96 Lichtjahre von der Sonne entfernten Hauptreihenstern 51 Eridani im Sternbild Eridanus umkreist.

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- [en] 51 Eridani b

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[ru] 51 Эридана b

51 Эридана b — юпитероподобная экзопланета, обращающаяся вокруг молодой звезды 51 Эридана, в созвездии Эридана[4]. Находится на расстоянии около 100 световых лет от Солнца. Её возраст около 20 млн лет[5].

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