Dynastic Vibes
The SMARTS 0.9-meter Telescope at Cerro-Tololo International Observatory (CTIO), a Program of NSF’s NOIRLab, has captured an echo of the past in this gorgeous Image of the Week. RCW 86 is a literal shell of its former self, the gaseous remnant of a supernova. Some 11,000 years ago a white dwarf, itself the core of a former star, became too massive and spectacularly exploded in a Type Ia supernova. Shockwaves reverberated through space, pushing the gas outward, whereupon it formed the multi-layered “bubble” we see today. Besides being a spectacular stellar object, the remnant may have been created by the earliest recorded supernova, observed by Chinese astronomers in 185 AD in the same area between the constellations Circinus and Centaurus.
Credit:CTIO/NOIRLab/NSF/AURA/T.A. Rector (University of Alaska Anchorage/NSF NOIRLab)
Image processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab) & D. de Martin (NSF NOIRLab)
About the Image
Id: | iotw2236a |
Type: | Observation |
Release date: | Sept. 7, 2022, noon |
Size: | 1723 x 2041 px |
About the Object
Wallpapers
Coordinates
Position (RA): | 14 40 19.60 |
Position (Dec): | -62° 39' 44.79" |
Field of view: | 11.53 x 13.65 arcminutes |
Orientation: | North is 179.6° left of vertical |
Colors & filters
Band | Wave-length | Tele-scope |
---|---|---|
Optical G | 475 nm | SMARTS–GSU 0.9-meter Telescope Tek2K |
Optical OIII | 502 nm | SMARTS–GSU 0.9-meter Telescope Tek2K |
Optical R | 626 nm | SMARTS–GSU 0.9-meter Telescope Tek2K |
Optical H-alpha | 656 nm | SMARTS–GSU 0.9-meter Telescope Tek2K |
Optical I | 773 nm | SMARTS–GSU 0.9-meter Telescope Tek2K |