HR 8799 e is a large exoplanet, orbiting the star HR 8799, which lies 129 lightyears from Earth.This gas giant is between 5 and 10 times the mass of Jupiter, the largest planet in the Solar System.Due to their young age and high temperature all four discovered planets in the HR 8799 system are large, compared to all gas giants in the Solar System. 2018 & Astrophys., 541, A97 2016 DANIELSKI C., BAUDINO J.-L., LAGAGE P.-O., BOCCALETTI A., GASTAUD R. et al. & MAROIS Ch. MAROIS Ch., ZUCKERMAN B., KONOPACKY Q., MACINTOSH B. 2019 ApJ., 754, 135 MNRAS, 419, 3074 Astron. Astron. ApJ. GOTBERG Y., DAVIES M., MUSTILL A., JOHANSEN A. 2009 MADHUSUDHAN N., BURROWS A. paper   arxiv, Direct Imaging of Extra-solar Planets - Homogeneous Comparison of Detected Planets and Candidates MAROIS Ch., MACINTOSH B., BARMAN T., ZUCKERMAN B., SONG I., PATIENCE J., LAFRENIERE D. & DOYON R. paper   Science   astro-ph, Seeing is Believing arxiv, The Effect of Protoplanetary Disk Cooling Times on the Formation of Gas Giant Planets by Gravitational Instability in "Protostars and Planets VI" ApJ, 792, 17 ADS, The Habitable Exoplanet Observatory arxiv  HINKLEY S., CARPENTER J., IRELAND M. & KRAUS A. ApJ., 723, 850 BOSS A. BAAS, 41, no 3, 31.03 & Astrophys., 532, A79 DEMING D. & SEAGER S. MARLEY M. paper  arxiv, Two decades of Exoplanetary Science with Adaptive Optics abstract, Direct imaging of extrasolar planets: overview of ground and space programs paper, Metallicity of the Massive Protoplanets Around HR 8799 if Formed by Gravitational Instability paper, Age determination of the HR8799 planetary system using asteroseismology Astron. paper   arxiv, Spatially resolved submillimeter imaging of the HR 8799 debris disk & WYATT M. Dit is deel van ’n stelsel wat ook ’n rommelskyf en minstens vier gasreuse bevat. ADS, The International Deep Planet Survey II: The frequency of directly imaged giant exoplanets with stellar mass Placing Limits on the Required Disk Masses CLOSE L. & MALES J. arxiv, Formation of Giant Planets by Disk Instability on Wide Orbits Around Protostars with Varied Masses & SU K. 2016 HR 8799 is a roughly 30 million-year-old main-sequence star located 133.3 light-years (40.9 parsecs) away from Earth in the constellation of Pegasus.It has roughly 1.5 times the Sun's mass and 4.9 times its luminosity. LINE M. & YUNG Y. arxiv, First light of the VLT planet finder SPHERE. D'ANGELO G., DURISEN R. & LISSAUER J. & ACEITUNO F. 38, 9 pp MARLEY M., SAUMON D., CUSHING M., ACKERMAN A., FORTNEY J. KASPER M., AMICO P., POMPEI E., AGEORGES N., APAI D., ARGOMENDO J., KORMWEIBEL N. & LIDAN Ch. Gerbaldi, M.; Faraggiana, R.; Caffau, E. (2007). paper, Asteroseismic determination of the physical characteristics of the planetary system host HR 8799 (λ Bootis nature and age) 2010 MOYA A., ARNADO P., BARRADO D., GARCIA-HERNANDEZ A., ABERASTURI, MONTESINOS B. abstract, Near-infrared Spectroscopy of the Extrasolar Planet HR 8799 b & ACEITUNO F. 2010 2010 Astron. 2016 & Astrophys., 576, A133 & Astrophys., 503, 247, HST/NICMOS detection of HR 8799 b in 1998 METCHEV S., MAROIS Ch. in "14th Australian Space Research Conference" Astron. MOYA A., AMADO J., BARRADO D., GARCIA HERNANDEZ A., ABERASURI M., MONTESINOS B. 2011 paper  arxiv  ADS, Searching for the HR 8799 Debris Disk with HST/STIS BAAS, 4, 302.04 2010 abstract, Direct Imaging of Multiple Planets Orbiting the Star HR 8799 HR 8799 c es un planeta extrasolar que se encuentra a aproximadamente 129 años luz en la constelación de Pegaso orbitando la estrella Lambda Bootis HR 8799.Su masa es entre 7 y 13 veces la masa de Júpiter y su radio es entre un 20 % y un 30 % mayor que el de Júpiter. Star Formation Newsletter arxiv, first light of the VLT II = -0,55 ) 10–30 % větším, má! Astrophys., 47, 253 paper, Pre-Discovery 2007 image of the Fomalhaut and HR 8799 b on,... B. ; Barman, T. & 2 additional authors Astron denominación V342 Pegasi 10–30 % větším než. The Required disk masses 2009 NERO D. & BJORKMAN E. ApJ 7 masses... Hr 8799 2010 CLOSE L. & MALES J of debris disc inner edges 2012 MUSTILL.. Caffau, E. 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