Explanation: Planets condense from disks. Several new Hubble Space Telescope pictures of stars surrounded by disks were released earlier this week. Since the glare of the central star usually makes a surrounding disk hard to see, prior observations in radio and infrared light were used to isolate systems where the disk was edge-on, blocking much of the central starlight. One such disk system, Haro 6-5B, is shown above in false color. Here, the central disk confines the emitted light into an hourglass shape. Complex dust clouds appear dark. A powerful protruding jet is shown in green. This budding planetary system measures 0.2 light-years across. Quite possibly, our own Solar System looked like this about 5 billion years ago.

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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: disk - jet - pylevoi disk - dzhet Publikacii so slovami: disk - jet - pylevoi disk - dzhet
Sm. takzhe: Porfirion: samyi dlinnyi dzhet ot chernoi dyry Galaktika, dzhet i znamenitaya chernaya dyra Akkreciruyushaya chernaya dyra s dzhetom HH 211: dzhety ot formiruyusheisya zvezdy Pylevoi disk vokrug Fomal'gauta Zvezdy, pyl', stolby i strui v tumannosti Pelikan Dzhet ot molodoi zvezdy MHO 2147 Vse publikacii na tu zhe temu >>