124-132
One of 42 new proplyds discovered in the Orion Nebula, 124-132 is one of the bright proplyds that lies relatively close to the nebula’s brightest star, Theta 1 Orionis C. This proplyd is surrounded by a shock wave that is caused by stellar wind from the massive Theta 1 Orionis C interacting with gas in the nebula.
Credit:NASA/ESA and L. Ricci (ESO)
About the Image
| Id: | heic0917as |
| Type: | Observation |
| Release date: | 14 December 2009, 16:00 |
| Related releases: | heic0917 |
| Size: | 128 x 128 px |
About the Object
| Name: | 124-132, Messier 42, Orion Nebula |
| Type: | Milky Way : Star : Circumstellar Material : Disk : Protoplanetary Milky Way : Nebula : Type : Star Formation |
| Distance: | 1400 light years |
| Category: | Nebulae |
Colours & filters
| Band | Wavelength | Telescope |
|---|---|---|
| Optical B | 435 nm |
Hubble Space Telescope
ACS |
| Optical V | 555 nm |
Hubble Space Telescope
ACS |
| Optical R | 775 nm |
Hubble Space Telescope
ACS |
| Optical H-alpha | 658 nm |
Hubble Space Telescope
ACS |