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Model of Fomalhaut b Dust Cloud
Hubble Captures Protoplanetary Collision in the Fomalhaut Star System
This diagram simulates what astronomers, studying Hubble Space Telescope observations, taken over several years, consider evidence for the first-ever detection of the aftermath of a titanic planetary collision in another star system. The color-tinted Hubble image on the left is of a vast ring of icy debris encircling the star Fomalhaut, located 25 light-years away. The star is so brilliant that a black occulting disk is used to block out its glare so that the dust ring can be photographed. In 2008, astronomers saw what they thought was the first direct image of a planet orbiting far from the star. However, by 2014, the planet candidate faded below Hubble's detection. The best interpretation is that the object wasn't ever a fully formed planet at all, but an expanding cloud of dust from a collision between two minor bodies, each about 125 miles across. The diagram at the right is based on a simulation of the expanding and fading cloud. The cloud, made of very fine dust particles, is currently estimated to be over 200 million miles across. Smashups like this are estimated to happen around Fomalhaut once every 200,000 years. Therefore, Hubble was looking at the right place at the right time to capture this transient event.
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.22:57:39.04
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.-29:37:20.04
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Piscis Austrinus
- DistanceDistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.The Fomalhaut star system is located 25 light-years away from Earth.
About the Data
- Data DescriptionData DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator. - InstrumentInstrumentThe science instrument used to produce the data.STIS/CCD
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.May 2012
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Fomalhaut b
- Object DescriptionObject DescriptionThe type of astronomical object.Model of Fomalhaut b expanding dust cloud
- Release DateApril 20, 2020
- Science ReleaseExoplanet Apparently Disappears in Latest Hubble Observations
- Credits
This image is a composite of many separate exposures made by the STIS instrument on the Hubble Space Telescope. This image was originally black and white and recorded only overall brightness. These brightness values were translated into a range of reddish hues. Such color "maps" can be useful in helping to distinguish subtly varying brightness in an image. Red: STIS/CCD.

Related Images & Videos
Illustration of Collision of Protoplanetary Bodies in the Fomalhaut Star System
This artist's illustration depicts the collision of two 125-mile-wide icy, dusty bodies orbiting the bright star Fomalhaut, located 25 light-years away. Astronomers believe that Hubble Space Telescope observations, spanning several years, provide observational evidence for the...

Model of Fomalhaut b Expanding Dust Cloud
Hubble Movie Captures Protoplanetary Collision in the Fomalhaut Star System This video simulates what astronomers, studying Hubble Space Telescope observations, consider evidence for the first-ever detection of the aftermath of a titanic planetary collision in another star...
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov