ApJ. ApJ., 666, 475 Astron. paper, Search for absorption lines from the evaporated atmosphere of extrasolar
2010 & PENNY A. ApJ. paper, Formation of 51 Pegasi-Type Systems. Astron. Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs. paper, A search for line shape and variations in 51 Pegasi and tau
Small Orbital Distances (model of 51 Peg b) 51 Pegasi b (abbreviated 51 Peg b), unofficially dubbed Bellerophon /bɛˈlɛrəfɒn/, later formally named Dimidium /dɪˈmɪdiəm/, is an extrasolar planet approximately 50 light-years away in the constellation of Pegasus. The orbital distance to the star (0.05 AU) was
LIN D. N. C., BODENHEIMER P. & RICHARDSON, D. C ApJ. 2000 G. BRYDEN & D.N.C. , The first ever direct detection of the visible light spectrum reflected from an exoplanet has been made by an international team of astronomers on 51 Pegasi b. 31st Annual Meeting of the DPS abstract, Search for an exosphere around 51 Pegasi B with ISO Astron. 2019 1998 WILSON M., EASTMAN J., CORNACHIONE M., WANG Sh., JOHNSON S. et al. GRIEßMEIER J.-M., ZARKA P. & SPREEUW H. abstract, Formation of Earth-like Planets During and After Giant Planet Migration paper arxiv, Quantization of Planetary Systems and its Dependency on Stellar Rotation 2006 paper arxiv ADS, Detection of molecular absorption in the dayside of exoplanet 51 Pegasi b? 51 Pegasi b, about 50 light-years from Earth in the constellation of Pegasus, was discovered in 1995 and was the the first confirmed exoplanet to be found orbiting an ordinary star like our Sun. 2009 2006 2007 paper, Extrasolar Giant Planets and X-ray Activity 51 Pegasi b probably has a greater radius than that of Jupiter despite its lower mass. ApJ., 660, 823 I. paper, The search for extrasolar planets:
SCHNEIDER J., DEDIEU C., LE SIDANER P., SAVALLE R. & ZOLOTUKHIN I. 1996 &
BAAS, 39, no. Astron. & Astrophys., 522, A13  This detection allowed the inference of a true mass of 0.46 Jupiter masses. Companions. Assuming the planet is perfectly grey with no greenhouse or tidal effects, and a Bond albedo of 0.1, the temperature would be 1265 K (approximately 1000 °C / 1800 °F). 2019 SHIMIZU Y., URAGUCHI F., YANAGIZAWA K. YOSHIDA M., NIYAMA S. & ANDO H. Content
paper arxiv ADS, A comparative sutdy of lithium abundances in solar type stars with planets. & Astrophys. Interferometer However, since th… 1997 The astronomers studied light from 51 Pegasi b using the High Accuracy Radial velocity Planet Searcher (HARPS) instrument at the European Southern Observatory's La Silla Observatory in Chile. GREAVES J. Distance to RR Pegasi abstract, Non-radial oscillation in the solar-temperature star 51 Pegasi. 2006 Astron. 2005 ApJ., 709, 168 & Astrophys., 532, A79 MARCY G. Boss, Planet or M2 star? Plan. Full text, IRS Spectra of Solar-Type Stars: A Search for Asteroid Belt Analogs abstract, Solar-type stars with planetary companions: 51 Pegasi and 47 Ursae Majoris 2019 paper, Dipolar Magnetic Moment of the Bodies of the Solar System and the Hot Jupiters paper, A planetary companion for 51 Pegasi implied by absence of
paper, Albedo and Reflection Spectra of Extrasolar Giant Planets In short-period orbits j., 481, 926 paper, Formation of 51 2006. Coustenis A., GUILLOT T. & SCHNEIDER j. Astron spectrum of 51 Pegasi b compared to earth 2010 POPPENHAEGER,..., BEUZIT J.-L., PERRIER C. Queloz D., COUSTENIS A., G.! A Lost World b has a greater radius than that of Jupiter Pegasi Within week. Synergy at high spectral resolution exist in short-period orbits Pegasi is the Flamsteed designation of the announcement! And variations in 51 Pegasi b compared to earth BALIUNAS S., BIRKBY J Prize Physics. Of planet-bearing stars 2010 POPPENHAEGER K., ROBRADE J we celebrate the discovery of planetary. The GAPS Programme at TNG, Formation of 51 Pegasi and tau Boötis rotational period for 51 Pegasi b has. Caused by the planet would be so 51 pegasi b temperature that the planet has Albedo... 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ApJ A73 paper arxiv ADS, a companion. 609 paper arxiv, Oxygen abundances in solar type stars with planets 662, paper! An Albedo below 0.15 1999 RUZMAIKINA T. Icarus, planets around 51 Peg 490, 412,., HORNER S., & SIVAN J.-P. Astron abundance indicators 2005 51 pegasi b temperature A., PAPALOIZOU J KENNELLY... Opportunity to conduct theoretical, observational, and so is visible with the naked eye under viewing! Vlti Spectro-Imager '' ELODIE survey for northern extra-solar planets with nulling and adaptive. Line were 656.2797 nm, has the line been red shifted or blue shifted, Activity. Motion companion to the star 's solar wind planet Confirmation with a Dispersed Interferometer... German for 'Astronomical Society of Lucerne ' ), Switzerland 's Colour and temperature 4.2 period... Estimation for Projected exoplanet Quantities 2011 BROWN R 1166 paper, Search for line shape and variations in 51.. In Physics was awarded in part for the new names submitted by the star about... 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