Discover Magazine on MSN
Hubble discovers Dracula’s Chivito, the largest-known chaotic planet nursery
Learn more about IRAS 23077+6707, a protoplanetary disk, nicknamed Dracuala's Chivito, that may serve as a planet nursery and ...
Morning Overview on MSN
Astronomers reveal the largest eccentric planet-forming disk ever seen
Astronomers have unveiled the largest planet-forming disk ever observed around a young star, a sprawling structure where gas ...
Roughly 1,000 light-years away from Earth, a gigantic disk of gas and dust is swirling around a young star and giving rise to ...
Green Matters on MSN
NASA Scientists Discover Largest Protoplanetary Disk Ever Seen Around a Young Star
Dracula's Chivito was detected by NASA’s Hubble Space Telescope and is located about 1,000 light-years from Earth.
Dracula's Chivito is the largest protoplanetary disk ever observed circling a young star, located at a distance of 1,000 ...
10don MSN
The chaotic 'Dracula's Chivito': Hubble reveals largest birthplace of planets ever observed
Astronomers using NASA's Hubble Space Telescope have imaged the largest protoplanetary disk ever observed circling a young ...
Space.com on MSN
'Dracula's Chivito' looks stunning in this tasty Christmas photo from the Hubble Telescope
"Hubble has given us a front row seat to the chaotic processes that are shaping disks as they build new planets — processes ...
Astronomers may have caught the first stages of planets being born around infant stars. The team discovered previously unseen rings, spirals and other substructures in the swirling, plate-like ...
NASA’s Hubble captured images of IRAS 23077+6707, the largest known protoplanetary disk, revealing its structure, asymmetry, and potential for forming multiple gas giant planets.
Archival ALMA data revealed a large, expanding bubble near the protoplanetary disk of the young star WSB 52, located approximately 441 light-years away. The bubble's formation is hypothesized to ...
Many newly formed stars are surrounded by what are called protoplanetary disks, swirling masses of warm dust and gas that can constitute the core of a developing solar system. Proof of the existence ...
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