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 • Nebulae Images/Videos |
| Distance: | 1400 light years |
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 |
