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X-ray Image of Galaxy Cluster MS 0735
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.07h 41m 50.2s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.74° 14' 51.0"
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Camelopardalis
- 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.About 2.6 billion light years
- DimensionsDimensionsThe physical size of the object or the apparent angle it subtends on the sky.4 arcminutes (3 million light-years or 900 kiloparsecs) wide
About the Data
- InstrumentInstrumentThe science instrument used to produce the data.CXO>ACIS
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.November 30, 2003
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.MS 0735.6+7421, Galaxy Cluster MS 0735
- Object DescriptionObject DescriptionThe type of astronomical object.Galaxy Cluster
- Release DateNovember 2, 2006
- Science ReleaseHost Galaxy Cluster to Largest Known Radio Eruption
- CreditNASA/CXC, B. McNamara (University of Waterloo and Ohio University)
CXO: X-ray
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Galaxy Cluster MS 0735
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Radio Image of Galaxy Cluster MS 0735
This radio image of galaxy cluster MS 0735.6+7421 was taken by NRAO's Very Large Array (VLA) in October 2004. The radio image shows jets of high energy particles ejected from a supermassive black hole, which is buried in the middle of the large central galaxy. The jets created...
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov
