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Abell 370 Parallel Field with Asteroids
Like rude relatives who jump in front your vacation snapshots of landscapes, some of our solar system's asteroids have photobombed deep images of the universe taken by NASA's Hubble Space Telescope. These asteroids reside, on average, only about 160 million miles from Earth — right around the corner in astronomical terms. Yet they've horned their way into this picture of thousands of galaxies scattered across space and time at inconceivably farther distances.
This Hubble photo of a random patch of sky is part of a survey called Frontier Fields. The colorful image contains thousands of galaxies, including massive yellowish ellipticals and majestic blue spirals. Much smaller, fragmentary blue galaxies are sprinkled throughout the field. The reddest objects are most likely the farthest galaxies, whose light has been stretched into the red part of the spectrum by the expansion of space.
Intruding across the picture are asteroid trails that appear as curved or S-shaped streaks. Rather than leaving one long trail, the asteroids appear in multiple Hubble exposures that have been combined into one image. Of the 20 total asteroid sightings for this field, seven are unique objects. Of these seven asteroids, only two were earlier identified. The others were too faint to be seen previously.
The trails look curved due to an observational effect called parallax. As Hubble orbits around Earth, an asteroid will appear to move along an arc with respect to the vastly more distant background stars and galaxies.
This parallax effect is somewhat similar to the effect you see from a moving car, in which trees by the side of the road appear to be passing by much more rapidly than background objects at much larger distances. The motion of Earth around the Sun, and the motion of the asteroids along their orbits, are other contributing factors to the apparent skewing of asteroid paths.
All the asteroids were found manually, the majority by "blinking" consecutive exposures to capture apparent asteroid motion. Astronomers found a unique asteroid for every 10 to 20 hours of exposure time.
The Frontier Fields program is a collaboration among NASA's Great Observatories and other telescopes to study six massive galaxy clusters and their effects. Using a different camera, pointing in a slightly different direction, Hubble photographed six so-called "parallel fields" at the same time it photographed the massive galaxy clusters. This maximized Hubble's observational efficiency in doing deep space exposures. These parallel fields are similar in depth to the famous Hubble Deep Field, and include galaxies about four-billion times fainter than can be seen by the human eye.
This picture is of the parallel field for the galaxy cluster Abell 370. It was assembled from images taken in visible and infrared light. The field's position on the sky is near the ecliptic, the plane of our solar system. This is the zone in which most asteroids reside, which is why Hubble astronomers saw so many crossings. Hubble deep-sky observations taken along a line-of-sight near the plane of our solar system commonly record asteroid trails.
The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, Inc., in Washington, D.C.
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.02:40:18.823
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.-01:36:12.269
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Cetus
- 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.4 billion light-years (to Abell 370)
- DimensionsDimensionsThe physical size of the object or the apparent angle it subtends on the sky.Image is 1 arcmin across (about 1.16 million light-years at distance of Abell 370)
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.Abell 370 is part of the Frontier Fields Program. These data are from the HST proposals 11108 (PI: E. Hu, University of Hawaii), 11507 (PI: K. Noll, GSFC), 11591 (PI: J.-P. Kneib, Laboratoire d'Astrophysique de Marseille), 13459 (PI: T. Treu, UCLA), 13790 (PI: S. Rodney, JHU), 14038 (PI: J. Lotz, STScI), and 14216 (R. Kirshner, Harvard University). For more information, see http://www.stsci.edu/hst/campaigns/frontier-fields. - InstrumentInstrumentThe science instrument used to produce the data.HST ACS/WFC; WFC3/IR
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.September 2009 - February 2015
- FiltersFiltersThe camera filters that were used in the science observations.ACS/WFC: F435W, F606W, and F814W; WFC3/IR: F105W, F125W, F140W, and F160W
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Abell 370 Parallel Field
- Object DescriptionObject DescriptionThe type of astronomical object.Asteroids in Foreground of Hubble Frontier Fields Image
- Release DateNovember 2, 2017
- Science ReleaseHubble Sees Nearby Asteroids Photobombing Distant Galaxies
- Credit
This image is a composite of separate exposures made by the WFC3 instrument on the Hubble Space Telescope using two different cameras and filters isolating the light of specific elements or of specific broad wavelength ranges. The color arises by assigning different hues (colors), to each monochromatic image. In this case, the colors are: blue WFC3/UVIS F435W + F606W, green WFC3/UVIS F814W + WFC3/IR F015W, orange/red WFC3/IR F125W + F140W + F160W.

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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov