File:RCW 120.jpg

Da testwiki.
Vai alla navigazione Vai alla ricerca
File originale (3 600 × 3 600 pixel, dimensione del file: 1,25 MB, tipo MIME: image/jpeg)

Questo file proviene da Wikimedia Commons e può essere utilizzato da altri progetti. Di seguito viene mostrata la descrizione presente nella pagina di descrizione del file.

Descrizione
English: Named RCW 120, this region of hot gas and glowing dust can be found in the murky clouds encircled by the tail of the constellation Scorpius. The ring of dust is actually glowing in infrared colors that our eyes cannot see, but show up brightly when viewed by Spitzer's infrared detectors. At the center of this ring are a couple of giant stars whose intense ultraviolet light has carved out the bubble, though they blend in with other stars when viewed in infrared.

The green ring is where dust is being hit by winds and intense light from the massive stars. The green color represents infrared light coming from tiny dust grains called polycyclic aromatic hydrocarbons. These small grains have been destroyed inside the bubble. The red color inside the ring shows slightly larger, hotter dust grains, heated by the massive stars.

This bubble is far from unique. Just as the Guardians of "Oa" have selected many beings to serve as Green Lanterns and patrol different sectors of space, Spitzer has found that such bubbles are common and an can be found around O stars throughout our Milky Way galaxy. The small objects at the lower right area of the image may themselves be similar regions seen at much greater distances across the galaxy.

Rings like this are so common in Spitzer's observations that astronomers have even enlisted the help of the public to help them find and catalog them all. Anyone interested in joining the search as a citizen scientist can visit "The Milky Way Project," part of the "Zooniverse" of public astronomy projects, at http://www.milkywayproject.org/.

RCW 120 can be found slightly above the flat plane of our galaxy, located toward the bottom of the picture. The green haze seen here is the diffuse glow of dust from the galactic plane.

This is a three-color composite that shows infrared observations from two Spitzer instruments. Blue represents 3.6-micron light and green shows light of 8 microns, both captured by Spitzer's infrared array camera. Red is 24-micron light detected by Spitzer's multiband imaging photometer.
Data
Fonte JPL-Caltech
Autore NASA/JPL-Caltech/GLIMPSE-MIPSGAL Teams
Licenza
(Riusare questo file)
Public domain Questo file è nel pubblico dominio perché creato dalla NASA. La politica sul copyright della NASA afferma che «il materiale della NASA non è protetto da copyright a meno che non sia specificato altrimenti». (NASA copyright policy e JPL Image Use Policy).
Attenzione:
Questa immagine o filmato è stato catalogato dal
Jet Propulsion Lab
della
National Aeronautics and Space Administration
(NASA) degli Stati Uniti d'Americacon il Photo ID: PIA14104 ET Alternate ID: sig11-007.

Questo tag non indica lo status del copyright dell'opera ad esso associato. È quindi richiesto un normale tag di copyright. Vedi Commons:Licenze per maggiori informazioni.
Altre lingue:

Didascalie

Aggiungi una brevissima spiegazione di ciò che questo file rappresenta

Elementi ritratti in questo file

raffigura

image/jpeg

Cronologia del file

Fare clic su un gruppo data/ora per vedere il file come si presentava nel momento indicato.

Data/OraMiniaturaDimensioniUtenteCommento
attuale00:33, 17 giu 2011Miniatura della versione delle 00:33, 17 giu 20113 600 × 3 600 (1,25 MB)wikimediacommons>Liandrei{{Information |Description={{en|1=Named RCW 120, this region of hot gas and glowing dust can be found in the murky clouds encircled by the tail of the constellation Scorpius. The ring of dust is actually glowing in infrared colors that our eyes cannot see

La seguente pagina usa questo file: