The Ghost Nebula
IC 63 — nicknamed the Ghost Nebula — is about 550 light-years from Earth. The nebula is classified as both a reflection nebula — as it is reflecting the light of a nearby star — and as an emission nebula — as it releases hydrogen-alpha radiation. Both effects are caused by the gigantic star Gamma Cassiopeiae. The radiation of this star is also slowly causing the nebula to dissipate.
Credit:ESA/Hubble, NASA
About the Image
| Id: | heic1818a |
| Type: | Observation |
| Release date: | 25 October 2018, 16:00 |
| Related releases: | heic1818 |
| Size: | 4072 x 4133 px |
About the Object
| Name: | IC 63 |
| Type: | Milky Way : Nebula : Appearance : Emission Milky Way : Nebula : Appearance : Reflection |
| Distance: | 600 light years |
| Constellation: | Cassiopeia |
| Category: | Nebulae |
Image Formats
Wallpapers
Coordinates
| Position (RA): | 0 59 7.75 |
| Position (Dec): | 60° 53' 59.35" |
| Field of view: | 2.69 x 2.73 arcminutes |
| Orientation: | North is 97.9° left of vertical |
View in ESASky:
View in WorldWide Telescope:
Colours & filters
| Band | Wavelength | Telescope |
|---|---|---|
| Ultraviolet UV | 275 nm |
Hubble Space Telescope
WFC3 |
| Optical g | 475 nm |
Hubble Space Telescope
WFC3 |
| Optical U | 336 nm |
Hubble Space Telescope
WFC3 |
| Optical r | 625 nm |
Hubble Space Telescope
WFC3 |
| Optical I | 814 nm |
Hubble Space Telescope
WFC3 |
| Infrared H | 1.6 μm |
Hubble Space Telescope
WFC3 |
| Infrared J | 1.1 μm |
Hubble Space Telescope
WFC3 |