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    JANSON M., CARSON J., LAFRENIERE D., SPIEGEL D., BENT J. This false-color composite image, taken with the Hubble Space Telescope, reveals the orbital motion of the planet Fomalhaut b. & STAPELFELDT K. 2014 Fomalhaut b had been identified as an exoplanet due to its features. 2006 paper  arxiv, A Primer on Unifying Debris Disk Morphologies Nature, 405, 1067 paper  arxiv, Discovery of the Fomalhaut C debris disc Astron. It has signed a contract to make this happen in 2025, Estée Lauder’s pricey goop gets seat on next ISS resupply mission as Japanese companies pledge zero-G cosmetics, Japan’s iSpace has put itself in the second column but also plans lunar landers of its own, Capsule tested atop Long March 5B can also get China to the Moon, £5m pot opened to biz and academics who fancy projects with foreign flavour, As Japan's virtual space tourism rig is readied for bolt-on to ISS, Combined Ministry of Defence and GCHQ team has worked since April to 'transform cyber capabilities', As the Interplanetary Networking Special Interest Group launches discussion of Solar System Internet. FARAMAZ V. paper  arxiv   RICCI L., TESTI L., MADDISON S. & WILNER D. RAMIREZ R. & KALTENEGGER L. Exoplanet. Astron. & Astrophys., 540, A125 paper, Fomalhaut's Debris Disk and Planet: Constraining the Mass of Fomalhaut b From Disk Morphology paper   arxiv, Herschel images of Fomalhaut - An extrasolar Kuiper belt at the height of its dynamical activity FARAMAZ V., BEUST H., AUGEREAU J.-Ch., KALAS P. & GRAHAM J. 2005 & Astrophys. 2016 LUBIN Ph. arxiv, Formation of Earth-like Planets During and After Giant Planet Migration paper, Numerical Modelling of Dusty Debris Disks. paper  arxiv, Light Scattering and Thermal Emission by Primitive Dust Particles in Planetary Systems LAWLER S., GREENSTREET S. & GLADMAN B. ApJ., 700, 1647 paper, Catalog of Nearby Exoplanets Over time, sharper images revealed an “Eye of Sauron” ring of warm dust encircling the star. The distant world — known as Fomalhaut b and located a neighborly 25 light-years from Earth — was infamous for being one of the first exoplanets ever discovered in visible light by NASA's Hubble Space Telescope; when astronomers first caught sight of it in 2004 and 2006, the planet appeared as a bright, cool dot moving briskly across the sky. 2009 2010 Its host star, Fomalhaut, is an A-type main-sequence star. Yet by 2014, the object had all but disappeared. Fomalhaut b, a directly imaged exoplanet This false-color composite image, taken with the Hubble Space Telescope, reveals the orbital motion of the planet Fomalhaut b. & AMARAA. abstract, The Hill stability of the possible moons of extrasolar planets 2007 ApJ., 625, 390, A planetary system as the origin of structure in Fomalhaut's dust belt. Fomalhaut b then began dimming, and by 2014 the telescope could no longer detect it. paper, The spin-orbit alignment of the Fomalhaut planetary system probed by optical long baseline interferometry ACKE B., MIN M., DOMINIK C., VANDENBUSSCHE B., SIBTHORPE B. (PhysOrg.com) -- Fomalhaut b, thought to be the first exoplanet photographed directly, has come under increased scrutiny due to evidence of an unexpected divergence from its … 2010 TAMAYO D. World's most comprehensive interactive database of extrasolar planets updated daily since 1995. When the exoplanet known as Fomalhaut b was first discovered, in the mid 2000s, it made history as one of the first worlds outside of our solar system to be seen directly. DONNISON J. 2017 2018 BEUST H., BONNEFOY M., MAIRE A.-L., EHRENREICH D., LAGRANGE A.-M. & CHAUNVIN G. 2012 Michael Perryman KENWORTHY M., MESHKAT T., QUANZ S., GIRARD J., MEYER M. & KASPER M. WHITE J., BOLEY A., DENT W., FORD E. & CORDER S. MNRAS, 473, 470 paper   arxiv, Coronagraphic observations of Fomalhaut at solar system scales ApJ. MENNESSON B., ABSIL O., LEBRETON J., AUGERAU J.-Ch., SERABYN E. & 5 additional authors Although originally thought to be a massive exoplanet, the faintness of Fomalhaut b in the infrared and its failure to perturb Fomalhaut’s debris ring indicate a low mass. 2012 2013 & Astrophys., 535, A68 arxiv, Clearing residual planetesimals by sweeping secular resonances in transitional disks: a lone-planet scenario for the wide gaps in debris disks around Vega and Fomalhaut paper, Did Fomalhaut, HR 8799, and HL Tauri Form Planets via the Gravitational Instability? abstract, How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits GRAHAM J., KALAS P., CHIANG E., FITZGERALD M., CLAMPIN M., KITE E., KRIST J. MANDELL A., RAYMOND S. & SIGURDSSON S. MNRAS, in press BAAS, 42, no 1, 377.07 The effect of an unseen inner mass on derived orbits paper   BUTLER P., WRIGHT J., MARCY G., FISCHER D., VOGT S., TINNEY Ch., JONES H., CARTER B., JOHNSON J., McCARTHY Ch. 2015 MNRAS, submitted Herschel images of Fomalhaut. MARCHI S. It is located approximately 25 light-years away in the Piscis Austrinus constellation. In November 2008, Hubble astronomers announced the exoplanet, named Fomalhaut b, as the first one ever directly imaged in visible light around another star. Astron. 2012 ApJ., 693, 734 MacGREGOR M., WILNER D., CHANDLER C., RICCI L., MADDISON S. et al. ApJ. Experts were left scratching their heads over the fate of Fomalhaut b, which appeared to orbit a bright star not too far from Earth. paper, Long range outward migration of giant planets, with application to Fomalhaut b 2015 & MAWET D. The bar shows a distance of 20 astronomical units, or 20 times the distance from the Sun to the Earth. paper, Insights on the dynamical history of the Fomalhaut system - Investigating the Fom c hypothesis ABSIL O. around Fomalhaut. MAMAJEK E. 2008 paper, Analysis of the Photometry of Fomalhaut b ApJ Letters, 760, L32 arxiv, A Complete ALMA Map of the Fomalhaut Debris Disk paper   arxiv, The Exoplanet Handbook 2013 ApJ, 764, 7 MATRA L., MACGREGOR M., KALAS P., WYATT M., KENNEDY G. et al. It is 1.9 times more massive and 1.8 times bigger compared with our Sun. arxiv, An interferometric study of the Fomalhaut inner debris disk. DELLER A. & 4 additional authors Suppl., 154, 458 arxiv, Extrasolar Kuiper Belts & PENNY A. paper, Giant Planet Formation 2015 paper   MNRAS, 448, 376 Astron. paper, Habitability of known exoplanetary systems based on measured stellar properties KALAS P., FITZGERALD M., PAPADOPOULOS P., GRAHAM J., MANESS H., MATTHEWS B., CLAMPIN M., CHIANG E. & BASU K. 2008 Astron. paper, The Ages of Stars Hosting Substellar Companions Its discovery was announced in 2008. paper  arxiv, Searching for faint companions with VLTI/PIONIER. KALAS P., GRAHAM J. paper, Predicting low-frequency radio fluxes of known extrasolar planets ApJ., 704, 150 & MADDISON S. It was clearly visible in several years of Hubble observations that revealed it as a moving dot. & MEGEATH S. 2006 arxiv   Fomalhaut b was labelled as one of the first exoplanets ever directly imaged by telescope. KENYON, S. & B. BROMLEY RILEY A., STRIGARI L., PORTER T., BLANDFORD R., MURGIA S. et al. paper  arxiv, Feasibility of transit photometry of nearby debris discs BOLEY A., PAYNE M., CORDER S., DENT W., FORD E. & SHABRAM M. paper   arxiv, Collisional Evolution of Irregular Satellite Swarms: Detectable Dust around Solar System and Extrasolar Planets paper  arxiv  ADS, 1.3 mm ALMA Observations of the Fomalhaut Debris System 2010 Fomalhaut b’s orbit was also odd and very eccentric. & Astrophys., 498, L41 The object, called Fomalhaut b, was first announced in 2008, based on data taken in 2004 and 2006. Rev., 18, 317 paper, First Look at the Fomalhaut Debris Disk with the Spitzer Space Telescope. BEUST H., AUGEREAU J.-Ch., BONSOR A., GRAHAM J., KALAS P. & 5 additional authors CATALDI G., BRANDEKER A., OLOFSSON G., CHEN C., DENT W. et al. paper   arxiv   ADS, A Possible Dynamical History for the Fomalhaut System Database query result: extrasolar planet systems ( of which are multiple planet systems) that contain total planets. & WONG P. & BROMLEY B. 2012 The host star Fomalhaut has apparent magnitude of 1.2, with absolute magnitude of 1.7. in IAU Symposium No. ApJ. Full text  arxiv   ADS. ApJ. G. Chauvin I. Near-infrared detection of hot dust with VLTI/VINCI 2017 Astron. The planet will appear to cross a vast belt of debris around the star roughly 20 years from now. ABSIL O., LE BOUQUIN J.-B., BERGER J.-Ph., LAGRANGE A.-M., CHAUVIN G. & 8 additional authors Now, a pair of academics at the University of Arizona in the US believe they have cracked it. JANSON M., WU Y., CATALDI G. & BRANDEKER A. Fomalhaut b’s orbit was also odd and very eccentric. paper  arxiv, Two decades of Exoplanetary Science with Adaptive Optics Scientists solve the mystery of the disappearing exoplanet Fomalhaut b. Shane McGlaun - Apr 21, 2020, 6:57am CDT. Detailed models of the exozodiacal disk and its origin & Astrophys., 640, A93 NEUHAEUSER R., HOHLE M., GINSKI Ch., SCHMIDT J., HAMBARYAN V. & SCHMIDT T. Image credit: Jason Wang/Paul Kalas; UC Berkeley. The reference to “20 au” means that the bar shows a distance of 20 astronomical units, or 20 times the distance from the sun to the Earth. Fomalhaut is the brightest star in the constellation Piscis Austrinus and lies 25 light-years away. 2014 KENWORTHY M., MAMAJEK E., HINZ Ph., MEYER M., HEINZE A., MILLER D., SIVANANDAM S. & FREED M. Instead, it’s actually a giant cloud of dust left over from the collision of two planetesimals that dispersed over time. 2015 GAUCHET L., LACOUR S., LAGRANGE A.-M., EHRENREICH D., BONNEFOY M. et al. JANSON M., QUANZ S., CARSON J., THALMANN Ch., LEFRENIERE D. & AMARA A. It is a class A star on the main sequence approximately 25 light-years from the Sun as measured by the Hipparcos astrometry satellite. The Case of the Disappearing Exoplanet Fomalhaut b was one of the first planets around another star to be directly imaged by telescopes. "Our study, which analyzed all available archival Hubble data on Fomalhaut revealed several characteristics that together paint a picture that the planet-sized object may never have existed in the first place," said András Gáspár, an assistant astronomer at the uni's Steward Observatory. Placing Limits on the Required Disk Masses paper   arxiv, Taxonomy of the extrasolar planet abstract, Direct imaging of extrasolar planets: overview of ground and space programs paper   arxiv, On the Age and Binarity of Fomalhaut Rev. 2016 PNAS, accepted ZEEGERS S., KENWORTHY M. & KALAS P. & Astrophys., 574, L1 MNRAS, 425, 2507 MIN M., KAMA M., DOMINIK C. & WATERS L. Astrobiology, 12, 361 paper   arxiv, Defining and cataloging exoplanets: The exoplanet.eu database 2015 2018 2012 paper, Optical to Submillimeter Imaging of the Fomalhaut and HR 8799 Planetary Systems. An artist's illustration of the disputed exoplanet Fomalhaut b. ABSIL O., MENNESSON B., LE BOUQIUN J.-B., DI FOLCO E., KERVELLA P. & AUGEREAU J.-Ch. Astron. SU K., RIEKE G., DEFRERE D., WANG K-S., LAI Sh.-P. et al. Fomalhaut b era, hasta ahora, uno de los pocos ejemplos de exoplaneta observado a través de imagen directa. 2011 The latest assessment reveals the object’s orbit isn’t elliptical; Fomalhaut b isn’t orbiting its host star – it’s actually on a path that will eventually lead it away from its star. 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. KIMURA H., KOLOKOLOVA L. LI A. 2009 2009 Fomalhaut b on its very long (1,700 year) and elliptica orbit, as seen here in five images taken by the Hubble Space Telescope over seven years. abstract, Fomalhaut b: Direct Detection of a less than 3 Jupiter-mass Object Orbiting Fomalhaut Fomalhaut b as a Dust Cloud: Frequent Collisions within the Fomalhaut Disk 2015 LAWLER S., GREENSTREET S. & GLADMAN B. ApJ Letters, 802, L20 2007 WYATT M. III. Known orbital times for exoplanets vary from a few hours (for those closest to their star) to thousands of years. MARLEY M. 2014 JONES B., SLEEP P. & UNDERWOOD D. paper, Imaged sub-stellar companions: not as eccentric as they appear? & Astrophys., 573, A87 arxiv   Content and Chapter 5, Are debris disks self-stirred? Astron. 2014 2013 ApJ, submitted Astron. paper   arxiv   ADS, Kinematics of planet-host stars and their relation to dynamical streams in the solar neighbourhood & Astrophys., 561, A43 Astron. 2009 POPPENHAEGER K., AUCHETTI K. & WOLK S. arxiv  in " Light Scattering Reviews, Volume 11", accepted BAAS, 41, no 1, 351.03 & ZHANG X. 314 "Young Stars & Planets Near the Sun" Entire South Carolina police force resigns, blames the mayor for backdoor… (Jason Wang/Paul Kalas; UC Berkeley) They believe Fomalhaut b was created after two objects about 125 miles (200 km) across smashed into one another not too long before it was first observed by Hubble in 2004. “These collisions are exceedingly rare and so this is a big deal that we actually get to see one We believe that we were at the right place at the right time to have witnessed such an unlikely event with NASA's Hubble Space Telescope," said Gáspár. "The Fomalhaut system is the ultimate test lab for all of our ideas about how exoplanets and star systems evolve,” George Rieke, co-author of the study and a professor of astronomy at the University of Arizona. MNRAS arxiv, Constraints on Planetesimal Collision Models in Debris Disks Part of Situation Publishing, Biting the hand that feeds IT © 1998–2020, No, really.

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