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APOD: 2024 November 17 B LDN 1471: A Windblown Star Cavity
<< Yesterday 17.11.2024
APOD: 2024 November 17 B LDN 1471: A Windblown Star Cavity
Credit & Copyright: Hubble, NASA, ESA; Processing & License: Judy Schmidt
Explanation: What is the cause of this unusual parabolic structure? This illuminated cavity, known as LDN 1471, was created by a newly forming star, seen as the bright source at the peak of the parabola. This protostar is experiencing a stellar outflow which is then interacting with the surrounding material in the Perseus Molecular Cloud, causing it to brighten. We see only one side of the cavity -- the other side is hidden by dark dust. The parabolic shape is caused by the widening of the stellar-wind blown cavity over time. Two additional structures can also be seen either side of the protostar; these are known as Herbig-Haro objects, again caused by the interaction of the outflow with the surrounding material. What causes the striations on the cavity walls, though, remains unknown. The featured image was taken by NASA and ESABs Hubble Space Telescope after an original detection by the Spitzer Space Telescope.

Explore Your Universe: Random APOD Generator

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: stellar wind - Herbig-Haro object
Publikacii so slovami: stellar wind - Herbig-Haro object
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