Cepheid Variable Star in Galaxy M100
This NASA/ESA Hubble Space Telescope image of a region of the galaxy M100 shows a class of pulsating star called a Cepheid Variable. Though rare, these stars are reliable distance indicators to galaxies. Based on the Hubble observation, the distance to M100 has been measured accurately as 56 million light-years (+/- 6 million light-years), making it the farthest object where intergalactic distances have been determined precisely.
Credit:About the Image
About the Object
| Name: | Messier 100 |
|---|---|
| Type: | Local Universe : Star : Type : Variable Local Universe : Galaxy : Type : Spiral |
| Distance: | 50 million light years |
| Constellation: | Coma Berenices |
| Category: | Galaxies Stars |
Classic Wallpapers
Coordinates
| Position (RA): | 12 23 0.55 |
|---|---|
| Position (Dec): | 15° 49' 22.16" |
| Field of view: | 2.52 x 1.80 arcminutes |
| Orientation: | North is 164.7° right of vertical |
View in ESASky:
View in WorldWide Telescope:
Colours & filters
| Band | Telescope |
|---|---|
| Optical |
Hubble Space Telescope
WFPC2 |