TAMAYO D. Astron. Fomalhaut A je zvijezda mase 1,92 puta veće od Sunčeve, oko 1,84 puta većega je promjera, 16,6 puta većega sjaja i površinske temperature oko 8590 K. Patuljasta je zvijezda glavnog iza spektralne klase A3V. & MEGEATH S. NERO D. & BJORKMAN E. paper, Extrasolar planet taxonomy: a new statistical approach KENNEDY G., WYATT M., KALAS P., DUCHENE G., SIBTHORPE B. et al. 2015 GAUCHET L., LACOUR S., LAGRANGE A.-M., EHRENREICH D., BONNEFOY M. et al. MIN M., KAMA M., DOMINIK C. & WATERS L. ABSIL O., MENNESSON B., LE BOUQIUN J.-B., DI FOLCO E., KERVELLA P. & AUGEREAU J.-Ch. COULSON I. ROBSON E. & GEAR W. 2013 & Astrophys., 539, L6 & Astrophys., 555, A146 paper   arxiv, Capture of Irregular Satellites via Binary Planetesimal Exchange Reactions in Migrating Planetary Systems OPPENHEIMER B. 2015). It is 1.9 times more massive and 1.8 times bigger compared with our Sun. 2010 DONNISON J. Ann. 2013 arxiv, STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b ApJ., 646, 505 ApJ Letters, 760, L32 paper   arxiv   ADS, A Possible Dynamical History for the Fomalhaut System CRIDA A., MASSET F. & MORBIDELLI A. Fomalhaut b est de 115 UA de son étoile, qui est environ dix fois la distance Saturne du soleil. & Astrophys., 574, L1 MENNESSON B., ABSIL O., LEBRETON J., AUGERAU J.-Ch., SERABYN E. & 5 additional authors ApJ., 693, 734 2005 2010 & LEBRETON J. Fomalhaut b, formellement Fomalhaut Ab, est une planète confirmée [5], [6] en orbite autour de l'étoile Fomalhaut A. Elle est la première exoplanète à avoir été détectée au moyen d'une photographie optique.La photographie, prise par le télescope spatial Hubble est publiée le 13 novembre 2008.. MANDELL A., RAYMOND S. & SIGURDSSON S. Its estimated surface temperature is 4,711 K and its luminosity only 0.19 L ☉. NEUHAEUSER R., HOHLE M., GINSKI Ch., SCHMIDT J., HAMBARYAN V. & SCHMIDT T. ADS, A Roadmap to Interstellar Flight 2013 ApJ., 666, 475 paper  arxiv, Optimized Principal Component Analysis on Coronagraphic Images of the Fomalhaut System 2013 ApJ., 582, 5821141 paper, The Ages of Stars Hosting Substellar Companions paper, An interferometric study of the Fomalhaut inner debris disk. 2009 JANSON M., QUANZ S., CARSON J., THALMANN Ch., LEFRENIERE D. & AMARA A. 2016 The star's effective temperature is 8,399 Kelvin which is hotter than our own Sun's effective Temperature which is 5,777 Kelvin. 2010 & Astrophys. paper  arxiv, Feasibility of transit photometry of nearby debris discs ZEEGERS S., KENWORTHY M. & KALAS P. We present new optical coronagraphic data of Fomalhaut obtained with HST/STIS in 2010 and 2012.Fomalhaut b is recovered at both epochs to high significance. 115 a.u. 2010 Astron. Fomalhaut b, one of the closest exoplanets at just 25.1 light-years distant, orbits within the edge of a debris disk (planetesimals?) Astron. ABSIL O., LE BOUQUIN J.-B., BERGER J.-Ph., LAGRANGE A.-M., CHAUVIN G. & 8 additional authors 2004 ApJ. arxiv, Constraints on Planetesimal Collision Models in Debris Disks arxiv   paper, Habitability of known exoplanetary systems based on measured stellar properties Letters, 750, L21 2009 I. & Astrophys., 535, A68 MNRAS, 448, 376 ACKE B., MIN M., DOMINIK C., VANDENBUSSCHE B., SIBTHORPE B. LAWLER S., GREENSTREET S. & GLADMAN B. arxiv, Consequences of an Eccentric Orbit for Fomalhaut b Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs. ECUVILLON A., ISRAELIAN G., PONT F., SANTOS N. & MAYOR M. 2005 If the planet's orbit lies in the same plane with the belt, icy and rocky debris in the belt could crash into the planet's atmosphere and produce various phenomena. NEUHAUSER R. & SCHMIDT T. 2008 2016 2014 ApJ, 823, 6 2007 ApJ., 747, 116 SAFFE C., LEVATO H., LOPEZ-GARCIA Z., JOFRE E., PETRUCCI R. & GONZALEZ E. paper, First Look at the Fomalhaut Debris Disk with the Spitzer Space Telescope. Recent studies have shown that both TW Piscis Austrini’s age of 450 million years, and its proper motion is consistent with the star being a true companion star. paper  arxiv, Searching for faint companions with VLTI/PIONIER. If not the first object identified through direct imaging — a brown dwarf failed star preceded it, as well as other objects that remain planet candidates — Fomalhaut …
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