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Compass and Scale Image for Galaxy Cluster SDSS J1110+6459, Lensed Galaxy SGAS J111020.0+645950.8
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.11h10m24.4s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.+64º59'16"
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Ursa Major
- 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.Galaxy cluster SDSS J1110+6459: 6.14 billion light years, lensed galaxy SGAS J111020.0+645950.8 11.05 billion light years
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.The Hubble image was created from HST data from proposal 13003 M. Gladders (U. Chicago) - InstrumentInstrumentThe science instrument used to produce the data.HST WFC3/UVIS, WFC3/IR
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.Jan. 8, 2013
- FiltersFiltersThe camera filters that were used in the science observations.WFC3/UVIS F390W, F606W, WFC3/IR F105W, F160W
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Galaxy cluster SDSS J1110+6459, lensed galaxy SGAS J111020.0+645950.8
- Object DescriptionObject DescriptionThe type of astronomical object.Galaxy cluster and gravitationally lensed galaxies
- Release DateJuly 6, 2017
- Science ReleaseHubble Pushed Beyond Limits to Spot Clumps of New Stars in Distant Galaxy
- 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 F390W, green WFC3/UVIS F606W, orange/red: WFC3/IR F105W, red WFC3/IR F160W.
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Details
Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov
