Credit & Copyright: JesZs M.Vargas & Maritxu Poyal
Explanation:
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).
Its distance is not well known but has been
estimated by some to be about 4,000 light-years.
Follow APOD on:
Facebook,
Google Plus,
Instagram, or
Twitter
1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 |
Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr' |
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 - NGC 6537 - Planetarnaya tumannost'
Publikacii so slovami: planetary nebula - NGC 6537 - Planetarnaya tumannost' | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
