Herbig-Haro Objects 76 and 77
A close-up of two Herbig-Haro (HH) objects found in the Circinus West molecular cloud: HH 76 (above center of image) and HH 77 (lower left). HH objects are glowing red patches of nebulosity commonly found near newborn stars. They form when fast-moving gas thrown out by stars smashes into slower-moving gas in the surrounding molecular cloud or interstellar medium. This image was taken with the Department of Energy-fabricated 570-megapixel Dark Energy Camera (DECam) — one of the most powerful digital cameras in the world — mounted on the U.S. National Science Foundation Víctor M. Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of NSF NOIRLab.
Credit:CTIO/NOIRLab/DOE/NSF/AURA
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Kosari (NSF NOIRLab)
About the Image
Id: | noirlab2515c |
Type: | Observation |
Release date: | April 24, 2025, 2 p.m. |
Related releases: | noirlab2515 |
Size: | 1080 x 1080 px |
About the Object
Wallpapers
Coordinates
Position (RA): | 15 0 39.69 |
Position (Dec): | -63° 5' 32.72" |
Field of view: | 5.27 x 5.27 arcminutes |
Orientation: | North is 0.1° left of vertical |
Colors & filters
Band | Wave-length | Tele-scope |
---|---|---|
Optical g | 473 nm | Víctor M. Blanco 4-meter Telescope DECam |
Optical g | 473 nm | Víctor M. Blanco 4-meter Telescope DECam |
Optical I | 784 nm | Víctor M. Blanco 4-meter Telescope DECam |
Optical I | 784 nm | Víctor M. Blanco 4-meter Telescope DECam |
Optical N662 | 662 nm | Víctor M. Blanco 4-meter Telescope DECam |