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The Lynx Arc: Stretched, Magnified Light From a Supercluster of Blue-White Stars
This NASA Hubble Space Telescope image of the Lynx cluster of galaxies shows the doubled image of the red Lynx arc (just right of the center). The mysterious arc is really a distant megacluster of stars lying far behind the galaxy cluster in the northern constellation Lynx.
The arc is the stretched and magnified image of a 12 billion light-year distant star-forming region. This remote source existed when the universe was less than 2 billion years old.
The discovery of this unique and puzzling object was the result of a systematic study of distant clusters of galaxies carried out with major X-ray, optical and infrared telescopes, including the Hubble Space Telescope, ROSAT and the Keck Telescopes.
The Hubble image, taken in deep red light with the Wide Field and Planetary Camera 2, has been color-enhanced using six ground-based images ranging from the blue to the infrared. Those six images were taken with the Mayall 4-meter Telescope at the National Optical Astronomy Observatory's Kitt Peak Observatory in Arizona.
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.08h 48m 48.76s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.44° 55' 49.6"
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Lynx
- 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.Approximately 12 billion light-years (4 billion parsecs)
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 object was imaged by Hubble during proposals 7374: P. Rosati (ESO), C. Norman, C. Mihos (CWRU), M. Dickinson, M. Giavalisco, and D. Macchetto (STScI) and proposal 8269: R. Elston (U. Florida), P. Eisenhardt, (JPL/Caltech), and A. Stanford (LLNL). The science team studying the arc is made up of: R. Fosbury (ST-ECF), M. Villar-Martín and A. Humphrey (U. Hertfordshire, UK), M. Lombardi and P. Rosati (ESO), D. Stern (LLNL), R. Hook (STScI), B.Holden and A. Stanford (UC Davis), G. Squires (SIRTF/Caltech), M. Rauch (Obs. of the Carnegie Inst. of Washington), W. L. W. Sargent (Caltech). - InstrumentInstrumentThe science instrument used to produce the data.HST>WFPC2
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.April 1999 and January-April 2000, Exposure Time: 8 hours
- FiltersFiltersThe camera filters that were used in the science observations.F702W (R), F814W (I)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Lynx arc
- Object DescriptionObject DescriptionThe type of astronomical object.Gravitational Lens
- Release DateOctober 30, 2003
- Science ReleaseMegastar-Birth Cluster is Biggest, Brightest and Hottest Ever Seen
- CreditsESA, NASA, Robert A.E. Fosbury (European Space Agency/Space Telescope-European Coordinating Facility, Germany) and NOAO
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov