The Lynx arc is a vast star birth region 12 billion light-years from Earth that contains 1 million ultra-hot stars. This artist's impression depicts torrent of ultraviolet radiation illuminating cold hydrogen gas. Astronomers regard this super star-birth region as an example of the early days of the universe where furious firestorms of star birth blazed across the skies.
Credits
Artwork
ESA, NASA, Robert A.E. Fosbury (ST-ECF)
| About The Object | |
|---|---|
| Object Name | Lynx arc |
| Object Description | Super star-birth region |
| R.A. Position | 08:48:48.76 |
| Dec. Position | +44:55:49.6 |
| Constellation | Lynx |
| Distance | 12 billion light-years (3.68 parsecs) |
| About The Object | |
|---|---|
| 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. |
