Fichier:Young Stars Emerge from Orion's Head.jpg
Fichier d’origine (3 182 × 1 282 pixels, taille du fichier : 4,21 Mio, type MIME : image/jpeg)
Ce fichier et sa description proviennent de Wikimedia Commons.
Description
DescriptionYoung Stars Emerge from Orion's Head.jpg |
English: This image from NASA's Spitzer Space Telescope shows infant stars "hatching" in the head of the hunter constellation, Orion. Astronomers suspect that shockwaves from a supernova explosion in Orion's head, nearly three million years ago, may have initiated this newfound birth.
The region featured in this Spitzer image is called Barnard 30. It is located approximately 1,300 light-years away and sits on the right side of Orion's head, just north of the massive star Lambda Orionis. Wisps of green in the cloud are organic molecules called polycyclic aromatic hydrocarbons (PAHs). PAHs are formed anytime carbon-based materials are burned incompletely. On Earth, they can be found in the sooty exhaust from automobile and airplane engines. They also coat the grills where charcoal-broiled meats are cooked. Tints of orange-red in the cloud are dust particles warmed by the newly forming stars. The reddish-pink dots at the top of the cloud are very young stars embedded in a cocoon of cosmic gas and dust. Blue spots throughout the image are background Milky Way along this line of sight. This composite includes data from Spitzer's infrared array camera instrument, and multiband imaging photometer instrument. Light at 4.5 microns is shown as blue, 8.0 microns is green, and 24 microns is red. |
Date | |
Source | http://www.spitzer.caltech.edu/images/2129-sig07-007-Young-Stars-Emerge-from-Orion-s-Head |
Auteur | NASA/JPL-Caltech/D. Barrado y Navascués (LAEFF-INTA) |
Image use policy: http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
Conditions d’utilisation
Public domainPublic domainfalsefalse |
Ce fichier provient de la NASA. Sauf exception, les documents créés par la NASA ne sont pas soumis à copyright. Pour plus d'informations, voir la politique de copyright de la NASA. | ||
Attention :
|
Éléments décrits dans ce fichier
dépeint
17 mai 2007
Historique du fichier
Cliquer sur une date et heure pour voir le fichier tel qu'il était à ce moment-là.
Date et heure | Vignette | Dimensions | Utilisateur | Commentaire | |
---|---|---|---|---|---|
actuel | 14 juin 2011 à 22:07 | 3 182 × 1 282 (4,21 Mio) | Spitzersteph |
Utilisation du fichier
La page suivante utilise ce fichier :
Métadonnées
Ce fichier contient des informations supplémentaires, probablement ajoutées par l'appareil photo numérique ou le numériseur utilisé pour le créer.
Si le fichier a été modifié depuis son état original, certains détails peuvent ne pas refléter entièrement l'image modifiée.
Largeur | 3 182 px |
---|---|
Hauteur | 1 282 px |
Schéma de compression | LZW |
Composition des pixels | RVB |
Titre de l’image | This image from NASA's Spitzer Space Telescope shows infant stars "hatching" in the head of the hunter constellation, Orion. Astronomers suspect that shockwaves from a supernova explosion in Orion's head, nearly three million years ago, may have initiated this newfound birth.
The region featured in this Spitzer image is called Barnard 30. It is located approximately 1,300 light-years away and sits on the right side of Orion's head, just north of the massive star Lambda Orionis. Wisps of green in the cloud are organic molecules called polycyclic aromatic hydrocarbons (PAHs). PAHs are formed anytime carbon-based materials are burned incompletely. On Earth, they can be found in the sooty exhaust from automobile and airplane engines. They also coat the grills where charcoal-broiled meats are cooked. Tints of orange-red in the cloud are dust particles warmed by the newly forming stars. The reddish-pink dots at the top of the cloud are very young stars embedded in a cocoon of cosmic gas and dust. Blue spots throughout the image are background Milky Way along this line of sight. This composite includes data from Spitzer's infrared array camera instrument, and multiband imaging photometer instrument. Light at 4.5 microns is shown as blue, 8.0 microns is green, and 24 microns is red. |
Orientation | Normale |
Nombre de composantes | 3 |
Résolution horizontale | 300 pt/po |
Résolution verticale | 300 pt/po |
Arrangement des données | Format tronçonné |
Logiciel utilisé | Adobe Photoshop CS3 Macintosh |
Date de modification du fichier | 5 juin 2009 à 14:36 |
Auteur | Spitzer Space Telescope |
Détenteur des droits d’auteur | http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml |
Espace colorimétrique | Non calibré |