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|  Message 10197  |
|  Alan Ianson to All  |
|  Daily APOD Report  |
|  19 Feb 25 00:13:12  |
 
MSGID: 1:153/757.0 a60eb9b9
TZUTC: -0800
CHRS: LATIN-1 2
Astronomy Picture of the Day
Discover the cosmos! Each day a different image or photograph of our
fascinating universe is featured, along with a brief explanation
written by a professional astronomer.
2025 February 19
A dark field has a single, colorful, blurry structure in its center.
Red-colored jets extend out from the center toward the top and bottom
of the frame. A dark disk covers the center. Blue outflows appear on
both sides of the horizontal disk. To the lower left, a larger blue
outflow extends. Please see the explanation for more detailed
information.
HH 30: A Star System with Planets Now Forming
Image Credit: James Webb Space Telescope, ESA, NASA & CSA, R. Tazaki et
al.
Explanation: How do stars and planets form? New clues have been found
in the protoplanetary system Herbig-Haro 30 by the James Webb Space
Telescope in concert with Hubble and the Earth-bound ALMA. The
observations show, among other things, that large dust grains are more
concentrated into a central disk where they can form planets. The
featured image from Webb shows many attributes of the active HH-30
system. Jets of particles are being expelled vertically, shown in red,
while a dark dust-rich disk is seen across the center, blocking the
light from the star or stars still forming there. Blue-reflecting dust
is seen in a parabolic arc above and below the central disk, although
why a tail appears on the lower left is currently unknown. Studying how
planets form in HH 30 can help astronomers better understand how
planets in our own Solar System once formed, including our Earth.
Tomorrow's picture: M87
__________________________________________________________________
Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
NASA Official: Amber Straughn Specific rights apply.
NASA Web Privacy, Accessibility, Notices;
A service of: ASD at NASA / GSFC,
NASA Science Activation
& Michigan Tech. U.
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