
This image shows the concentration of starlight at the core of merging galaxy cluster Abell 520. The map was derived from observations by the Canada-France-Hawaii Telescope in Hawaii.
Abell 520 resides 2.4 billion light-years away.
Credits
NASA, ESA, CFHT, M.J. Jee (University of California, Davis), and A. Mahdavi (San Francisco State University)About The Object | |
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Object Name | Abell 520 |
Object Description | Merging Galaxy Cluster |
R.A. Position | 04h 54m 18.98s |
Dec. Position | 02° 56' 48.8" |
Constellation | Orion |
Distance | 2.4 billion light-years (740 million parsecs) |
About The Data | |
Data Description | CFHT (B) |
Instrument | CFHT |
Filters | CFHT (B) |
About The Image | |
Color Info | Orange: CFHT (B) |
About The Object | |
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Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
Object Description | The type of astronomical object. |
R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
Distance | The 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. |
Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
About The Data | |
Data Description |
|
Instrument | The science instrument used to produce the data. |
Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
Filters | The camera filters that were used in the science observations. |
About The Image | |
Image Credit | The primary individuals and institutions responsible for the content. |
Publication Date | The date and time the release content became public. |
Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |