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Affichage des articles dont le libellé est ASTRONOMY - LDN 1471: A Windblown Star Cavity. Afficher tous les articles
Affichage des articles dont le libellé est ASTRONOMY - LDN 1471: A Windblown Star Cavity. Afficher tous les articles

17/11/2024

ASTRONOMY - LDN 1471: A Windblown Star Cavity

 2024 November 17

A starfield is dominated by light brown dust. In the 
middle is a parabolic gas cloud opening toward the lower right.
A bright star is near the center at the apex of the parabolic
gas cloud. 
Please see the explanation for more detailed information.

LDN 1471: A Windblown Star Cavity
Image Credit: HubbleNASAESAProcessing & LicenseJudy 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 ESA’s Hubble Space Telescope after an original detection by the Spitzer Space Telescope.

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