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.

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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.

Publikacii s klyuchevymi slovami: Herbig-Haro object - planet formation - Ob'ekt Herbiga-Aro - Formirovanie planet Publikacii so slovami: Herbig-Haro object - planet formation - Ob'ekt Herbiga-Aro - Formirovanie planet
Sm. takzhe: HH 211: dzhety ot formiruyusheisya zvezdy Molodye zvezdy i dzhety Igra: krushenie superplanet HH 666: pylevoi stolb s dzhetom v Kile Dzhety v ob'ekte Herbiga-Aro 24 Dugi, dzhety i udarnye volny okolo NGC 1999 Molodye solnca v NGC 7129 Vse publikacii na tu zhe temu >>