Re: Terry's Astronomy Thread.
What's in the sky tonight?
October 29, 2012
Astro Picture of the Day:
October 29, 2012
Source:
Oh what a tangled web a planetary nebula can weave. The Red Spider Planetary Nebula shows the complex structure that can result when a normal star ejects its outer gases and becomes a white dwarf star. Officially tagged NGC 6537, this two-lobed symmetric planetary nebula houses one of the hottest white dwarfs ever observed, probably as part of a binary star system. Internal winds emanating from the central stars, visible in the center, have been measured in excess of 1000 kilometers per second. These winds expand the nebula, flow along the nebula's walls, and cause waves of hot gas and dust to collide. Atoms caught in these colliding shocks radiate light shown in the above representative-color picture by the Hubble Space Telescope. The Red Spider Nebula lies toward the constellation of the Archer (Sagittarius). It's distance is not well known but has been estimated by some to be about 4,000 light-years.
What's in the sky tonight?
October 29, 2012
-Full Moon (exact at 3:49 p.m. Eastern Daylight Time). Look a fist-width above the Moon for the brightest stars of Aries, lined up nearly horizontally.
-Algol should be at minimum light for a couple hours centered on 10:03 p.m. EDT.
-Jupiter's Great Red Spot (pale orange-tan) crosses Jupiter's central meridian around 11:32 p.m. Eastern Daylight Time.
-Algol should be at minimum light for a couple hours centered on 10:03 p.m. EDT.
-Jupiter's Great Red Spot (pale orange-tan) crosses Jupiter's central meridian around 11:32 p.m. Eastern Daylight Time.
Astro Picture of the Day:
October 29, 2012

Oh what a tangled web a planetary nebula can weave. The Red Spider Planetary Nebula shows the complex structure that can result when a normal star ejects its outer gases and becomes a white dwarf star. Officially tagged NGC 6537, this two-lobed symmetric planetary nebula houses one of the hottest white dwarfs ever observed, probably as part of a binary star system. Internal winds emanating from the central stars, visible in the center, have been measured in excess of 1000 kilometers per second. These winds expand the nebula, flow along the nebula's walls, and cause waves of hot gas and dust to collide. Atoms caught in these colliding shocks radiate light shown in the above representative-color picture by the Hubble Space Telescope. The Red Spider Nebula lies toward the constellation of the Archer (Sagittarius). It's distance is not well known but has been estimated by some to be about 4,000 light-years.


















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