
This is an image of the intricate remains of Supernova 1987A taken by NASA’s Chandra X-ray Observatory. The blue hue reveals where the expanding shock wave from the exploded star is colliding with a ring of material around the supernova. The blue color reveals the hottest gas.
NASA, ESA, and A. Angelich (NRAO/AUI/NSF)
Chandra image: NASA/CXC/Penn State/K. Frank et al.
Credits
Image
NASA, ESA, CXC, PSU, A. Angelich (NRAO, AUI, NSF), Kari Frank (PSU)
About The Object | |
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Object Name | SN 1987A |
Object Description | Supernova Remnant |
R.A. Position | 05h 35m 28.03s |
Dec. Position | -69° 16' 11".8 |
Constellation | Dorado |
Distance | Approximately 163,000 light-years (50 kiloparsecs) away |
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 |
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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. |