The distorted shape of this tiny object, called POX 186, is evidence that it is a dwarf galaxy in the process of formation. This image, obtained by NASA's Hubble Space Telescope, shows the bluish-white glow of newborn stars at the galaxy's core, and an arch of stars (at right). Both features suggest a recent collision between two smaller clumps of stars that occurred within the past 100 million years. Gravity will eventually pull these stars together into a more symmetrical form. The red objects at the edges of the images are most likely more distant galaxies.
The Hubble images reveal POX 186 to be extremely small by galaxy standards, measuring only about 900 light-years across and containing just 10 million stars. By contrast, the Milky Way galaxy is about 100,000 light-years across and contains over 100 billion stars.
The galaxy is 68 million light-years away in the constellation Virgo. This color image was created from a composite of three pictures obtained by the Wide Field and Planetary Camera 2 in March and June 2000, and approximates what the galaxy would look like to the human eye.
Credits
NASA and Michael Corbin (CSC/STScI)| About The Object | |
|---|---|
| Object Name | POX 186, PGC 046982 |
| Object Description | Dwarf Galaxy |
| R.A. Position | 13h 25m 49.99s |
| Dec. Position | -11° 37' 36.0" |
| Constellation | Virgo |
| Distance | About 21 megaparsecs (68,500,000 light-years) |
| Dimensions | This image is 12.7 arcseconds wide. At the distance to NGC 1705, this corresponds to roughly 1,300 parsecs (4,200 light-years). |
| About The Data | |
| Data Description | Principal Astronomers: M. Corbin (CSC/STScI) and W. Vacca (MPE, Garching) |
| Instrument | HST>WFPC2, and HST>STIS |
| Exposure Dates | March 15, 2000, Exposure Time: 2 hours (WFPC2), and June 16, 2000, Exposure Time: 1.2 hours (STIS) |
| Filters | WFPC2: F336W (U), F555W (V), F814W (I) STIS: G140L and G230L |
| About The Image | |
| Compass Image |  |
| 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. |
