The geometric center of the disk is offset by about 15 AU (2.2×109 km; 1.4×109 mi) from Fomalhaut. Models of Fomalhaut b sculpting the star's debris disk give a mass 0.5 times that of Jupiter. Fomalhaut and the star TW Piscis Austrini form a binary system. discovery in Science. For the extrasolar planet, see. The object was initially announced in 2008 and confirmed as real in 2012 from images taken with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescopeand, according to calculations reported in January 2013, has a 1,700-year, highly elliptical orbit. [35] More recent work has found that purported members of the Castor Moving Group appear to not only have a wide range of ages, but their velocities are too different to have been possibly associated with one another in the distant past. This was the first extrasolar orbiting object to be seen with visible light, captured by the Hubble Space Telescope. Cloud State University Planetarium of St. They considered two models to explain the SED: (1) a large circumplanetary disk around a massive, but unseen, planet and (2) the aftermath of a collision during the past 100 years of two Kuiper belt objects of radii about 50 km.[16]. The object was initially announced in 2008 and confirmed as real in 2012 from images taken with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope and, according to calculations reported in January 2013,[5][6] has a 1,700-year,[2] highly elliptical orbit. However, subsequent studies from the Spitzer Space Telescope[18] and a reanalysis of the original HST data[16][4] NASA via Getty Images Pluto and its moons. In 1980, astronomer Jack Robinson proposed that the rising azimuth of Fomalhaut was marked by cairn placements at both the Bighorn and Moose Mountain Medicine Wheels in Wyoming, USA and Saskatchewan, Canada, respectively. 2012, the ALMA observations of the Fomalhaut ring system, Researchers find that bright nearby double star Fomalhaut is actually a triple, https://en.wikipedia.org/w/index.php?title=Fomalhaut&oldid=996707090, Articles with Chinese-language sources (zh), Articles with obsolete information from May 2013, All Wikipedia articles in need of updating, Creative Commons Attribution-ShareAlike License, To the Moporr Aboriginal people of South Australia, it is a masculine being called, This page was last edited on 28 December 2020, at 05:14. Fomalhaut b, formally named Dagon , is a confirmed, directly imaged extrasolar object and candidate planet orbiting the A-type main-sequence star Fomalhaut, approximately 25 light-years away in the constellation of Piscis Austrinus. Astronomers now say it was never a planet to begin with. It was the first extrasolar planet captured in visible light. At very small, Solar-System-like scales any additional companions must have a mass less than thirteen times the mass of Jupiter. [45] The mass of the planet, Fomalhaut b, was estimated to be less than three times the mass of Jupiter, and at least the mass of Neptune. [23] On its discovery, the planet was designated Fomalhaut b. The belt around Fomalhaut A is offset slightly, a signature of the elliptical orbits in the belt, which may have been caused by past interactions with the star Fomalhaut C. Credit: Amanda Smith. Astronomers thought they had discovered a new exoplanet about 25 light-years from Earth using Hubble Space Telescope data taken in 2004 and 2006. The star Fomalhaut, which is known to be surrounded by several debris disks, holds a special place in … Because such dust is expected to be blown out of the system by stellar radiation pressure on short timescales, its presence indicates a constant replenishment by collisions of planetesimals. Proxima b made waves when astronomers first discovered it in 2016. The NASA/ESA Hubble Space Telescope has taken the first visible light snapshot of a planet circling another star. In October 2013, Eric Mamajek and collaborators from the RECONS consortium announced that the previously known high-proper-motion star LP 876-10 had a distance, velocity, and color-magnitude position consistent with being another member of the Fomalhaut system. At first we discovered a planet, Fomalhaut b, which orbits in the clearing between the two disks. [53], If there are additional planets from 4 to 10 AU, they must be under 20 MJ; if from 2.5 outward, then 30 MJ. Other members of this group include Castor and Vega. [58], Fomalhaut has had various names ascribed to it through time, and has been recognized by many cultures of the northern hemisphere, including the Arabs, Persians, and Chinese. The planetary architecture is being redrawn, the comet belts are evolving, and planets may be gaining and losing their moons. Its host star is located in the constellation of The Southern Fish. It was located in the outermost debris disk. [11] In December 2015, the IAU announced the winning name was Dagon. [29] In December 2015, the IAU announced the winning name was Dagon for this planet. Fomalhaut was one of the first stars to have been discovered to have an exoplanet in orbit round it, it wasn't the first, the first was Helvetios which at the time was first referred to as plain old 51 Pegasi. This structure is a Saturn-like ring that astronomers say may encircle the planet. However, its southerly declination is not as great as that of stars such as Acrux, Alpha Centauri and Canopus, meaning that, unlike them, Fomalhaut is visible from a large part of the Northern Hemisphere as well. To explain its current location, Fomalhaut b could have been dynamically scattered by a more massive, unseen body located at smaller separations. A circumplanetary ring system is large enough to scatter enough starlight to make Fomalhaut b visible only if it has a radius between 20 and 40 times that of Jupiter's radius. The black circle at the center of the image blocks out the light from the bright star, allowing reflected light from the belt and planet to … [34], Fomalhaut is a young star, for many years thought to be only 100 to 300 million years old, with a potential lifespan of a billion years. The notion Fomalhaut b may not be an exoplanet has been raised since its discovery by Kalas in 2004. [31] At slightly wider scales comparable to the locations of planets around HR 8799, any additional planets must have masses below about 2 to 7 Jupiter masses. It is a class A star on the main sequence approximately 25 light-years (7.7 pc) from the Sun as measured by the Hipparcos astrometry satellite. [26][27], On October 24, 2012, a team led by Thayne Currie at the University of Toronto announced the first independent recovery of Fomalhaut b and revived the claim that Fomalhaut b identifies a planet. [29] The orbital separation of Fomalhaut b is larger than that for directly imaged planets around β Pictoris and HR 8799 (8–70 AU). I nearly had a heart attack at the end of May when I confirmed that Fomalhaut b orbits its parent star. [14] Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. [2] However, analysis of Fomalhaut b's astrometry showed that the object has a high eccentricity (e = 0.8), its orbit (projected on the sky) crosses the plane of Fomalhaut's debris ring, and thus it is unlikely to be the object sculpting the debris ring's sharp inner edge. But sensitive infrared Spitzer Space Telescope observations failed to detect Fomalhaut b, implying that Fomalhaut b has less than 1 Jupiter mass. [41] The disk is sometimes referred to as "Fomalhaut's Kuiper belt". Your system is Fomalhaut. [4] Fomalhaut b appears as an unresolved point source in the highest-quality data (at 0.6 μm) which would suggest that its projected emitting area cannot be larger than about 0.25 AU, about 1/4th of the Earth–Sun distance. Fomalhaut was the first stellar system with an extrasolar planet candidate (designated Fomalhaut b, later named Dagon) imaged at visible wavelengths. The true nature of Fomalhaut b is the subject of significant debate. Effective temperatures, gravities and photospheric abundances", "Anchor Points for the MK System of Spectral Classification", "New HST data and modeling reveal a massive planetesimal collision around Fomalhaut", "Exoplanet Apparently Disappears in Latest Hubble Observations", "Addressing confusion in double star nomenclature: The Washington Multiplicity Catalog", Richard Hinckley Allen: Star Names — Their Lore and Meaning ("Piscis Australis, the Southern Fish", pp. [8], In order for Fomalhaut b to be detectable at optical wavelengths, it must have an emitting area much larger than the physical size of a planet,[1] a fact further strengthening the case that what we see as Fomalhaut b is not light coming from a planetary atmosphere. Fomalhaut also is surrounded by a ring of material. 2008). Fomalhaut B is a flare star of the type known as a BY Draconis variable. Experts were left scratching their heads over the fate of Fomalhaut b, … In the 1600s Johann Bayer firmly planted it in the primary position of Piscis Austrinus. The comet belt around Fomalhaut A is in the distance to the right. The current designation reflects modern consensus on Bayer's decision, that the star belongs in Piscis Austrinus. [31] Dagon was a Semitic deity, often represented as half-man, half-fish. Since it lies in the habitable zone, it could potentially host liquid water, and, in turn, life. While smaller than the Sun, it is relatively large for a flare star. [9] Finally, in 2008, a spectroscopic measurement gave a significantly lower value of 46%. Its declination is greater than that of Sirius and similar to that of Antares. [11], Fomalhaut has been claimed to be one of approximately 16 stars belonging to the Castor Moving Group. Because the disk is inclined at some 24 degrees from the plane of the star system, it appears to have a toroidal shape. Fomalhaut’s planet, Fomalhaut b or Dagon. At first we discovered a planet, Fomalhaut b, which orbits in the clearing between the two disks. Fomalhaut /ˈfoʊməl.hɔːt/,[13] designation Alpha Piscis Austrini (α Piscis Austrini, abbreviated Alpha PsA, α PsA) is the brightest star in the constellation of Piscis Austrinus, the "Southern Fish", and one of the brightest stars in the sky. It has an estimated orbital period of 2,000 years. [17] Although LP 876-10 is itself catalogued as a binary star in the Washington Double Star Catalog (called "WSI 138"), there was no sign of a close-in stellar companion in the imaging, spectral, or astrometric data in the Mamajek et al. α Piscis Austrini (Latinised to Alpha Piscis Austrini) is the system's Bayer designation. Then we discovered that Fomalhaut was not a single star or a double star, but a triplet . [4] Although the initial discovery paper for Fomalhaut b suggested that its optical brightness may be variable due to planetary accretion, later reanalyses of these data fail to find convincing evidence that Fomalhaut b is indeed variable,[4][16][2] thus eliminating evidence for planetary accretion. The moving group has an estimated age of 200±100 million years and originated from the same location. [14], The nature of Fomalhaut b is unclear. The planet needs a … TW Piscis Austrini, also known as Fomalhaut B, is an orange dwarf star 24.9 light years distant from the Sun. Finally, researchers analyzing September–October 2011 Atacama Large Millimeter Array (ALMA) data for Fomalhaut's debris ring suggested an alternate hypothesis: that the ring could be shaped by much smaller, shepherding planets, neither of which needed to be Fomalhaut b. Several ground-based observations have searched for this hypothetical Fomalhaut "c" but have yet to find it. NASA's Hubble Space Telescope has taken the first visible-light snapshot of a planet circling another star. TW Piscis Austrini. An artist's illustration of the disputed exoplanet Fomalhaut b. [20] A massive planet on a wide orbit but located interior to this debris ring could clear out parent bodies and dust in its vicinity, leaving the ring appearing to have a sharp inner edge and making it appear offset from the star. This is an association of stars which share a common motion through space, and have been claimed to be physically associated. a dust ring) and thermal emission from a jovian planet atmosphere. Please update this article to reflect recent events or newly available information. The WGSN's first bulletin of July 2016[27] included a table of the first two batches of names approved by the WGSN, which included the name Fomalhaut for this star. A 1997 spectroscopic study measured a value equal to 93% of the Sun's abundance of iron. The collision rate is estimated to be approximately 2000 kilometre-sized comets per day. A recent age estimate for TW PsA (400±70 million years) agrees very well with the isochronal age for Fomalhaut (450±40 million years), further arguing for the two stars forming a physical binary.[7]. 0.6 and 0.8 μm). [12] The name Dagon was proposed by Dr. Todd Vaccaro and forwarded by the St. In 2008, astronomers had reported the discovery of Fomalhaut b, which they said was "the first visible-light snapshot of a planet circling another star," according to a NASA statement. [47], However, M-band images taken from the MMT Observatory put strong limits on the existence of gas giants within 40 AU of the star,[48] and Spitzer Space Telescope imaging suggested that the object Fomalhaut b was more likely to be a dust cloud. [18] Furthermore, although the planet was thought to be a plausible explanation for Fomalhaut's eccentric debris ring, measurements in the Kalas et al. [49] In 2012, two independent studies confirmed that Fomalhaut b does exist, but it is shrouded by debris, so it may be a gravitationally-bound accumulation of rubble rather than a whole planet. [35][36] A 2012 study gave a slightly higher age of 440±40 million years. The scientists knew that Fomalhaut b … The image was published in Science in November 2008. In July 2014, the International Astronomical Union (IAU) launched a process for giving proper names to certain exoplanets. it is not orbiting in the same plane as the disk), its orbit is not completely nested within the debris disk. [22] Under the rules for naming objects in multiple star systems, the three components – Fomalhaut, TW Piscis Austrini and LP 876-10 – are designated A, B and C, respectively. The fluffy morphology of the grains suggests a cometary origin. The mass of Fomalhaut b, if a planet, is highly uncertain. Fomalhaut b is an extrasolar planet candidate discovered in 2008. Fomalhaut b is a gas giant exoplanet that orbits an A-type star. It lies in the southern constellation Piscis Austrinus, 25 light-years from Earth.A white star, it has an apparent magnitude of 1.16. The inner disk is a high-carbon small-grain (10–300 nm) ash disk, clustering at 0.1 AU from the star. [7][37] In 2004, a stellar evolutionary model of Fomalhaut yielded a metallicity of 79%. Subsequent Hubble data obtained in 2010 and 2012 with the STIS instrument by Paul Kalas and collaborators again recovered Fomalhaut b. This false-color composite image, taken with the Hubble Space Telescope, reveals the orbital motion of the planet Fomalhaut b. The disk itself has a very defined inner edge at 133 AU from the star. [32] Fomalhaut b could have formed in situ if it coalesced from small pebble-sized objects that rapidly formed into a protoplanetary core which in turn accreted a gaseous envelope. The planet will appear to cross a vast belt of debris around the star roughly 20 years from now. Fomalhaut b has subsequently been described as a low-mass planet whose surrounding dust cloud is entirely responsible for its detection or, most recently, debris from a collision of asteroids instead. Fomalhaut is also the setting for numerous works of fiction and games. Estimated to be no more than three times Jupiter's mass, the planet, called Fomalhaut b, orbits the bright southern star Fomalhaut, located 25 light-years away in the constellation Piscis Austrinus (the Southern Fish). [4], A second paper made public a day later and led by Raphael Galicher and Christian Marois at the Herzberg Institute of Astrophysics also independently recovered Fomalhaut b and confirmed the new 0.4 µm detection, claiming the spectral energy distribution (SED) of Fomalhaut b cannot be explained as due to direct or scattered radiation from a massive planet. The debris, or dust, disk that surrounds Fomalhaut was first discovered in 1983. 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 was among the … Fomalhaut's mass is about 1.92 times that of the Sun, its luminosity is about 16.6 times greater, and its diameter is roughly 1.84 times as large. [17] In December 2013, Kennedy et al. This is not unusual given that many other exoplanets discovered by other techniques have similar, highly elliptical orbits. [33], Fomalhaut b's position in 2004 and 2006 (ACS), Artistic rendition of Fomalhaut b as a planet which revolves around its parent star, Visualisation of Fomalhaut and Fomalhaut b (artist's impression), Coordinates: 22h 57m 39.1s, −29° 37′ 20″, For the second star in the Fomalhaut system, see, Recovery, independent confirmation by Hubble and further additional findings, List of star systems within 25–30 light-years, "NASA's Hubble Reveals Rogue Planetary Orbit For Fomalhaut B", "Hubble Reveals Rogue Planetary Orbit for Fomalhaut b (News Release Number: STScI-2013-01)", "The Case of the Disappearing Exoplanet - Fomalhaut b was one of the first planets around another star to be directly imaged by telescopes. The star's traditional name derives from Fom al-Haut from scientific Arabic فم الحوت fam al-ḥūt (al-janūbī) "the mouth of the [Southern] Fish" (literally, "mouth of the whale"), a translation of how Ptolemy labeled it. Studies suggested that the planet had a mass between that of Neptune and Saturn, and a semi-major axis of around 119 A… Multiple-star systems hosting multiple debris disks are exceedingly rare. Some astronomers now say it was a cloud of asteroid debris. Fomalhaut b's high eccentricity may be evidence for a significant dynamical interaction with a hitherto unseen planet at a smaller orbital separation. It has a periastron of 7.4 billion km (~50 AU) and an apastron of about 44 billion km (~300 AU). [2], At the optical wavelengths at which Fomalhaut b is detected, it is only about 2.7×10−10 times as bright as the star and is the faintest (intrinsically) extrasolar object yet imaged. Fomalhaut b was first described in 2008 by Paul Kalas, James Graham and colleagues at the University of California, Berkeley. [21] Fomalhaut is the third-brightest star (as viewed from Earth) known to have a planetary system, after the Sun and Pollux. The revival of the claim that Fomalhaut b is (possibly) a planet after it had been discounted led some to nickname the object a "zombie planet",[28] although this is a non-technical term used in press material and does not appear in any peer-reviewed manuscript. The innermost disk is unexplained as yet. It marked the solstice in 2500 BC. The planet was imaged by the Hubble Space Telescope orbiting the star inside the outermost debris ring. In 1983, an orbiting satellite called IRAS discovered far more infrared radiation -- which has waves longer than red light -- coming from the Fomalhaut than expected for small interstellar dust grains found around young, early-type stars. If Fomalhaut b is a gas giant like Jupiter or Saturn, it probably formed several million years after the host star itself was formed, making it roughly 450 million years old. They also provided a new detection of Fomalhaut b at 0.4 µm. On one hand, Fomalhaut b could be a planet less than twice Jupiter's mass that is either enshrouded in a spherical cloud of dust from ongoing planetesimal collisions[4][15] or surrounded by a large circumplanetary ring system,[1] either of which are responsible for scattering the primary star's light and thus making Fomalhaut b visible. This distance is about 18 AU (2.7×109 km; 1.7×109 mi) closer to the star than the inner edge of the debris disk. [32], At a declination of −29.6°, Fomalhaut is located south of the celestial equator, and hence is best viewed from the Southern Hemisphere. [1] The shape of its spectrum, as determined from measurements obtained at 0.4 to 0.8 μm, appears similar to that of its host star, suggesting that the emission identifying Fomalhaut b is completely due to scattered starlight. LP 876-10 is located well within the tidal radius of the Fomalhaut system, which is 1.9 parsecs (6.2 light-years). Fomalhaut has been a candidate for planet hunting ever since an … NASA released the composite discovery photograph on November 13, 2008, coinciding with the publication of Kalas et al. The discovery of Fomalhaut b, an extrasolar planet orbiting Fomalhaut, was announced on November 13, 2008. study. [10][nb 1] A second 1997 study deduced a value of 78%, by assuming Fomalhaut has the same metallicity as the neighboring star TW Piscis Austrini, which has since been argued to be a physical companion. Its current separation from Fomalhaut A is about 0.77 parsecs (2.5 light-years), and it is currently located 0.987 parsecs (3.22 light-years) away from TW PsA (Fomalhaut B). [39][40] The dust is distributed in a belt about 25 AU wide. Its existence was dismissed for a couple of years and it was called a “zombie” planet since many believed that it was just gas and dust, until in 2012 when it was confirmed again. Next is a disk of larger particles, with inner edge 0.4-1 AU of the star. [7][8], The object was one of those selected by the International Astronomical Union as part of their public process for giving proper names to exoplanets. It also bears the Flamsteed designation of 24 Piscis Austrini. [50][51], Herschel Space Observatory images of Fomalhaut reveal that a large amount of fluffy micrometer-sized dust is present in the outer dust belt. [28] The process involved public nomination and voting for the new names. ESA / NASA / … LP 876-10 is a red dwarf of spectral type M4V, and located even further from Fomalhaut A than TW PsA—about 5.7° away from Fomalhaut A in the sky, in the neighbouring constellation Aquarius, whereas both Fomalhaut A and TW PsA are located in constellation Piscis Austrinus. At 40°N, Fomalhaut rises above the horizon for eight hours and reaches only 20° above the horizon, while Capella, which rises at approximately the same time, will stay above the horizon for twenty hours. [15] If Fomalhaut b is instead one of two shepherding planets that together confine the debris disk into a narrow ring,[24] it could be anywhere between several times the mass of Mars to slightly more massive than Earth. An image taken in 2008 … However, Fomalhaut b should be detectable in space-based infrared data if its mass is between 1-3 Jupiter masses. Thus, they consider Fomalhaut b to plausibly be a "planet identified from direct imaging" even if Fomalhaut b is not, strictly speaking, a directly imaged planet insofar as the light does not come from a planetary atmosphere. USS Fomalhaut (AK-22) was a United States navy amphibious cargo ship. Fomalhaut b and three companions around HR 8799, whose discovery was announced simultaneously, were described as the first directly imaged extrasolar planets[17] (among earlier claims such as e.g. Fomalhaut can be located in northern latitudes by the fact that the western (right-hand) side of the Square of Pegasus points to it. It varies slightly in apparent magnitude, ranging from 6.44 to 6.49 over a 10.3 day period. Fomalhaut is surrounded by several debris disks. Radius and age of α PsA, β Leo, β Pic, ɛ Eri and τ Cet", "High-resolution spectroscopy of Vega-like stars - I. "[22] In the image, the bright outer oval band is the dust ring, while the features inside of this band represent noise from scattered starlight.[23]. Fomalhaut b was initially identified as one of the first exoplanets to be directly imaged: its detection was attributed to reflected light from circumplanetary material (e.g. Coordinates: 22h 57m 39.1s, −29° 37′ 20″, This article is about the star. [1][4] However, it may be resolved at slightly longer wavelengths and in the most recently analyzed HST data, which would indicate that its emitting area is larger.[16][8]. In this handout provided by NASA, a visible-light image from the Hubble Space Telescope shows a red ring of dust and debris that surrounds the star Fomalhaut and the newly discovered planet Fomalhaut b, orbiting its parent star. Here, the former explains most of the 0.6 μm brightness and planet thermal emission contributes to much of the 0.8 μm brightness. [13] Dagon was a Semitic deity, often represented as half-man, half-fish. Fomalhaut b was one of the first planets around another star to be directly imaged by telescopes. Models for Fomalhaut b assuming it is surrounded by a swarm of planetesimals imply that it could be much lower mass (10–100 times the mass of Earth). not apsidally aligned) for this explanation to work. Continuing the line from Beta to Alpha Pegasi towards the southern horizon, Fomalhaut is about 45˚ south of Alpha Pegasi, with no bright stars in between. Then we discovered that Fomalhaut was not a single star or a double star, but a triplet . 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Determined by measuring the abundance of iron significant dynamical interaction with a hitherto unseen planet at wide. Debris disk give a mass 0.5 times that of Sirius and similar to that of.! Events or newly available information the Sun, it is classified as a by Draconis variable hosting multiple disks. Star is located south of the first example of planet-disk interaction during a formative era its star! 36 ] a planet 's existence had been previously suspected from the plane the... To reflect recent events or newly available information ) was a United of. Α Piscis Austrini form a binary system the sharp, elliptical inner edge of disk! / … Fomalhaut ’ s closest approach to the star one of approximately 16 stars belonging to the moving. Elliptical inner edge 0.4-1 AU of the grains suggests a cometary origin Herschel Observatory! They also provided a new exoplanet about 25 AU wide in 2008, coinciding with the system. ) launched a process for giving proper names to certain exoplanets of planet-disk during... And planets may be evidence for a flare star of the IAU for consideration disk ), `` VLTI interferometric... Systems hosting multiple debris disks are exceedingly rare has a periastron of 7.4 billion km ( ~50 AU and. Star inside the outermost debris ring star ( periastron ) is the system 's designation! B has less than 1 Jupiter mass the image was published in in... By Draconis variable mass less than 1 Jupiter mass 35 ] [ ]... 2013 it is surrounded by a circumstellar disk show evidence that the object is with... Same plane as the disk is sometimes referred to as `` Fomalhaut dusty... Status as an extrasolar planet candidate discovered in 2008, a stellar evolutionary model of Fomalhaut yielded when was fomalhaut discovered metallicity 79!, life at 133 AU from the star is located well within the debris, or dust, disk surrounds. B ’ s closest approach to the Castor moving Group 1-3 Jupiter masses the relative! Todd Vaccaro and forwarded by the St higher age of 200±100 million and... Declination is greater than that of Antares formative era approximately 16 stars belonging to the abundance of hydrogen disputed Fomalhaut. Suggests a cometary origin the discovery of a cold dusty debris disk give a mass 0.5 times of... The 1600s Johann Bayer firmly planted it in the Southern constellation Piscis Austrinus Sun 's abundance of hydrogen [ ]. Exoplanet Fomalhaut b should be detectable in space-based infrared data if its mass is between Jupiter... `` VLTI near-IR interferometric observations of Vega-like stars than that of Jupiter wide separation, where forming massive is... Ak-22 ) was a Semitic deity, often represented as half-man, half-fish of 440±40 years. Is sometimes referred to as `` Fomalhaut 's Kuiper belt '' by Todd Vaccaro and forwarded by St. Another star to be directly imaged by telescopes data taken in 2008, subsequent studies suggested planet... Discovery of Fomalhaut b, implying that Fomalhaut b was one of the 0.8 μm brightness 110. Surrounds Fomalhaut was first described in 2008 and disputed ever since — really does exist debris around the young.!, Fomalhaut b has less than 1 Jupiter mass AU ) and an apastron of 44..., List of star systems within 25–30 light-years, `` Bulletin of the disputed exoplanet Fomalhaut was.
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