KuvausM27 Knots.jpg	Close up detail of knots in planetary nebula Messier 27
Päiväys	marraskuu 2001
Lähde	http://hubblesite.org/newscenter/archive/releases/2003/06/image/a (direct link)
Tekijä	C.R. O'Dell (Vanderbilt University)
Käyttöoikeus (Tämän tiedoston uudelleenkäyttö)	Public domainPublic domainfalsefalse Tämä teos on ilman tekijänoikeuden suojaa, koska National Aeronautics and Space Administration (NASA) loi sen. Koska Nasa on Yhdysvaltain liittovaltion organisaatio, sen luomat teokset ovat ilman tekijänoikeuden suojaa. ([1][2]) Varoitukset: Nasan logo ja insigniat eivät ole vapaasti käytettäviä. ([3]) Nasan Internet-sivustolla on paljon kuvia Neuvostoliiton avaruusohjelmasta, Venäjän avaruusjärjestöltä, Euroopan avaruusjärjestöltä (ESA) ja muilta avaruusjärjestöiltä tai viranomaisilta. Niiden kuvat eivät välttämättä ole tekijänoikeudesta vapaita. Hubble-teleskoopilla otetut kuvat saattavat olla tekijänoikeuden alaisia, jos ne eivät tule Space Telescope Science Institutelta (STScI). ([4]) Solar and Heliospheric Observatoryn (SOHO) kuvien käyttäminen muutoin kuin epäkaupallisesti tai opetuksellisesti vaatii luvan. ([5]) Astronomy Picture of the Day (APOD) -sivuston kuvat saattavat olla tekijänoikeuden alaisia. ([6])

Picture shows a 99″.5 × 75″.5 section of the central region of M 27.^[1]

From the NASA source site [7]:

An aging star's last hurrah is creating a flurry of glowing knots of gas that appear to be streaking through space in this close-up image of the Dumbbell Nebula, taken with NASA's Hubble Space Telescope.

The Dumbbell, a nearby planetary nebula residing more than 1,200 light-years away, is the result of an old star that has shed its outer layers in a glowing display of color. The nebula, also known as Messier 27 (M27), was the first planetary nebula ever discovered. French astronomer Charles Messier spotted it in 1764.

The Hubble images of the Dumbbell show many knots, but their shapes vary. Some look like fingers pointing at the central star, located just off the upper left of the image; others are isolated clouds, with or without tails. Their sizes typically range from 11 - 35 billion miles (17 - 56 billion kilometers), which is several times larger than the distance from the Sun to Pluto. Each contains as much mass as three Earths.

The knots are forming at the interface between the hot (ionized) and cool (neutral) portion of the nebula. This area of temperature differentiation moves outward from the central star as the nebula evolves. In the Dumbbell astronomers are seeing the knots soon after this hot gas passed by.

Dense knots of gas and dust seem to be a natural part of the evolution of planetary nebulae. They form in the early stages, and their shape changes as the nebula expands. Similar knots have been discovered in other nearby planetary nebulae that are all part of the same evolutionary scheme. They can be seen in Hubble telescope photos of the Ring Nebula (NGC 6720), the Eskimo Nebula (NGC 2392) and the Retina Nebula (IC 4406). The detection of these knots in all the nearby planetaries imaged by the Hubble telescope allows astronomers to hypothesize that knots may be a feature common in all planetary nebulae.

This image, created by the Hubble Heritage Team (STScI), was taken by Hubble's Wide Field Planetary Camera 2 in November 2001, by Bob O'Dell (Vanderbilt University) and collaborators. The filters used to create this color image show oxygen in blue, hydrogen in green and a combination of sulfur and nitrogen emission in red.

Object Names: Dumbbell Nebula, M27, NGC 6853

Image Type: Astronomical

Image Credit: NASA and The Hubble Heritage Team (STScI/AURA)

Acknowledgment: C.R. O'Dell (Vanderbilt University)

References