
The image on the left shows the GRB 971214 field, obtained with the W.M. Keck 10-meter telescope on Mauna Kea, Hawaii about two days after the burst. The image on the right was obtained with the Space Telescope Imaging Spectrograph (STIS) aboard the Hubble Space Telescope about four months later.
Credits
S. G. Djorgovski and S. R. Kulkarni (Caltech), the Caltech GRB Team, and W. M. Keck Observatory, and NASAAbout The Object | |
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Object Name | GRB 971214 |
R.A. Position | 11h 56m 30.0s |
Dec. Position | 65° 12' 0.0" |
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. |