- Tata Surya
- Epsilon Eridani b
- Abdullah Gymnastiar
- Daftar bintang di rasi bintang Eridanus
- Daftar bintang terdekat
- Daftar sistem multiplanet
- Daftar eksoplanet
- Daftar planet luar surya yang ditemukan pada tahun 2000–2009
- 51 Eridani
- 51 Eridani b
- Epsilon Eridani
- Delta Eridani
- Epsilon Eridani b
- List of directly imaged exoplanets
- HD 10647 b
- T dwarf
- Gemini Observatory
- List of stars in Eridanus
51 Eridani GudangMovies21 Rebahinxxi LK21
51 Eridani is a star in the constellation Eridanus. It has an apparent magnitude of 5.22, meaning it is just visible to the unaided eye in suburban and rural skies. The primary star's absolute magnitude is 2.87. There is also a binary star named GJ 3305 which shares the same proper motion through space with it, making it overall a triple star system.
General information
Johann Bayer gave the star its Bayer designation of c Eridani, using lowercase letters once he had exhausted all the letters of the Greek alphabet, in his 1603 star chart Uranometria. It was catalogued as 51 Eridani by John Flamsteed in 1725.
Located around 97 light-years distant, it shines with a luminosity approximately 5.72 times that of the Sun and has a surface temperature of 7,400 K. A cold debris disk has been detected with a likely inner border of 82 astronomical units (AU). A yellow-white main-sequence star of spectral type F0V, 51 Eridani is a member of the Beta Pictoris moving group and hence thought to be around 23 million years old. Somewhat more luminous than it should be for its surface temperature, 51 Eridani has also been classified as spectral type F0IV—a type corresponding to ageing stars that have used up their core hydrogen fuel and become subgiants; however, in this case it is a phenomenon of very young stars 5 to 30 million years old that have yet to settle on the main sequence.
Photometric measurements with the TESS space telescope show that this is a Gamma Doradus-like pulsating star. Nine pulsation frequencies have been detected.
= GJ 3305
=51 Eridani has a companion, known as GJ 3305. The system has a common proper motion with 51 Eridani, and hence it is gravitationally bound, although it is separated by 66″ corresponding to 2,000 AU. It is a binary star system with two M-type red dwarfs. The primary has a mass of 0.67 ± 0.05 M☉ while the secondary has a mass of 0.44 ± 0.05 M☉. The two red dwarfs themselves are separated by a semimajor axis of 9.78 ± 0.14 AU and have an eccentricity of 0.19 ± 0.02.
The star is significant as the host sun to one of the first planets to have been directly imaged in wide-orbit, and the first detected by the Gemini Planet Imager.
Planetary system
51 Eridani b is a young Jupiter-like planet and was photographed, in near-infrared light, on 21 December 2014. The study, led by Bruce Macintosh, a professor of physics at Stanford University and confirmed by Christian Marois found that methane and water were abundant in the atmosphere of the planet and its diameter was only slightly larger than Jupiter's. It is the smallest exoplanet directly imaged to date. The planetary orbit was found to be significantly eccentric by 2019.
Gaia astrometry also suggests an additional planet on orbit smaller than 51 Eridani b.
References
Cited text
Kata Kunci Pencarian:
Eridani - YouTube
51_Eridani_b – exocast
Eridani on Behance
Eridani on Behance
51 Eridani - Star in Eridanus | TheSkyLive.com
51 Eridani - Star in Eridanus | TheSkyLive.com
40 Eridani | Incoming call screenshot, Incoming call, Empire
40 Eridani B – Rochester Astronomy Club
40 Eridani B – Rochester Astronomy Club
EarthSky | 51 Eridani b: An exoplanet orbits its star
51 Eridani Ab | The Universe of The Universe Wiki | Fandom
51 Eridani b (artist's conception) | The Planetary Society