Explanation: It's a weed, it's Jupiter, no it's - actually planetary nebula NGC 3242. After a star like our Sun completes fusion in its core, it throws off its outer layers it a striking display called a planetary nebula. NGC 3242 is such a planetary nebula, with the stellar remnant white dwarf star visible at the center. This nebula is sometimes called "The Ghost of Jupiter" for its similar appearance to the familiar planet. NGC 3242 is much farther away however, than the measly 40 light-minutes distance to Jupiter. In fact, by comparing the apparent expansion rate with the actual rate determined from Doppler studies, astronomers have estimated the distance to NGC 3242 to be about 1400 light-years away. The red FLIERs visible near the edges of the nebula remain mysterious.

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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: planetary nebula - Planetarnaya tumannost' - Yupiter - Evolyuciya zvezd Publikacii so slovami: planetary nebula - Planetarnaya tumannost' - Yupiter - Evolyuciya zvezd
Sm. takzhe: Pogruzhenie v Yupiter Kometa, planeta, Luna Kol'ca vokrug tumannosti Kol'co Periiovii 16: proletaya nad Yupiterom Planety i polnoe zatmenie HFG1 i Eibell 6: planetarnye tumannosti Yupiter za 2 chasa 30 minut Vse publikacii na tu zhe temu >>