Fichier:Triple Jupiter Eclipse.jpg
Le contenu de la page n’est pas pris en charge dans d’autres langues.
Apparence
Taille de cet aperçu : 600 × 600 pixels. Autres résolutions : 240 × 240 pixels | 480 × 480 pixels | 900 × 900 pixels.
Fichier d’origine (900 × 900 pixels, taille du fichier : 49 kio, type MIME : image/jpeg)
Ce fichier et sa description proviennent de Wikimedia Commons.
Description
DescriptionTriple Jupiter Eclipse.jpg |
English: At first glance, Jupiter looks like it has a mild case of the measles. Five spots - one colored white, one blue, and three black are scattered across the upper half of the planet. Closer inspection by NASA's Hubble Space Telescope reveals that these spots are actually a rare alignment of three of Jupiter's largest moons - Io, Ganymede, and Callisto - across the planet's face. In this image, the telltale signatures of this alignment are the shadows [the three black circles] cast by the moons. Io's shadow is located just above center and to the left; Ganymede's on the planet's left edge; and Callisto's near the right edge. Only two of the moons, however, are visible in this image. Io is the white circle in the center of the image, and Ganymede is the blue circle at upper right. Callisto is out of the image and to the right. On Earth, we witness a solar eclipse when our Moon's shadow sweeps across our planet's face as it passes in front of our Sun. Jupiter, however, has four moons roughly the same size as Earth's Moon. The shadows of three of them occasionally sweep simultaneously across Jupiter. The image was taken March 28, 2004, with Hubble's Near Infrared Camera and Multi-Object Spectrometer. Seeing three shadows on Jupiter happens only about once or twice a decade. Why is this triple eclipse so unique? Io, Ganymede, and Callisto orbit Jupiter at different rates. Their shadows likewise cross Jupiter's face at different rates. For example, the outermost moon Callisto orbits the slowest of the three satellites. Callisto's shadow moves across the planet once for every 20 shadow crossings of Io. Add the crossing rate of Ganymede's shadow and the possibility of a triple eclipse becomes even more rare. Viewing the triple shadows in 2004 was even more special, because two of the moons were crossing Jupiter's face at the same time as the three shadows. Jupiter appears in pastel colors in this photo because the observation was taken in near-infrared light. Astronomers combined images taken in three near-infrared wavelengths to make this color image. The photo shows sunlight reflected from Jupiter's clouds. In the near infrared, methane gas in Jupiter's atmosphere limits the penetration of sunlight, which causes clouds to appear in different colors depending on their altitude. Studying clouds in near-infrared light is very useful for scientists studying the layers of clouds that make up Jupiter's atmosphere. Yellow colors indicate high clouds; red colors lower clouds; and blue colors even lower clouds in Jupiter's atmosphere. The green color near the poles comes from a thin haze very high in the atmosphere. Ganymede's blue color comes from the absorption of water ice on its surface at longer wavelengths. Io's white color is from light reflected off bright sulfur compounds on the satellite's surface. In viewing this rare alignment, astronomers also tested a new imaging technique. To increase the sharpness of the near-infrared camera images, astronomers speeded up Hubble's tracking system so that Jupiter traveled through the telescope's field of view much faster than normal. This technique allowed scientists to take rapid-fire snapshots of the planet and its moons. They then combined the images into one single picture to show more details of the planet and its moons. |
Date | |
Source | https://flic.kr/p/93mnhZ (see also http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=3083) |
Auteur | NASA, ESA, and E. Karkoschka (University of Arizona) |
Autres versions |
|
Cette image ou vidéo a été cataloguée par l’un des centres de la National Aeronautics and Space Administration (NASA) des États-Unis sous Photo ID : SPD-SLRSY-3083.Ce bandeau n’indique rien sur le statut de l’œuvre au regard du droit d'auteur. Un bandeau de droit d’auteur est requis. Voir Commons:À propos des licences pour plus d’informations. Autres langues :
العربية ∙ беларуская (тарашкевіца) ∙ български ∙ català ∙ čeština ∙ dansk ∙ Deutsch ∙ English ∙ español ∙ فارسی ∙ français ∙ galego ∙ magyar ∙ հայերեն ∙ Bahasa Indonesia ∙ italiano ∙ 日本語 ∙ македонски ∙ മലയാളം ∙ Nederlands ∙ polski ∙ português ∙ русский ∙ sicilianu ∙ slovenščina ∙ Türkçe ∙ українська ∙ 简体中文 ∙ 繁體中文 ∙ +/− |
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 :
|
This image was originally posted to Flickr by NASA on The Commons at https://flickr.com/photos/44494372@N05/5277461005. It was reviewed on 2017-08-03 20:38:57 by FlickreviewR, who found it to be licensed under the terms of the No known copyright restrictions, which is compatible with the Commons. It is, however, not the same license as given above, and it is unknown whether that license ever was valid. |
Éléments décrits dans ce fichier
dépeint
domaine public<\/a>"}},"text\/plain":{"fr":{"P6216":"domaine public"}}}}" class="wbmi-entityview-statementsGroup wbmi-entityview-statementsGroup-P6216 oo-ui-layout oo-ui-panelLayout oo-ui-panelLayout-framed">
28 mars 2004
image/jpeg
m\u00e9thode de d\u00e9termination<\/a>"}},"text\/plain":{"fr":{"":"m\u00e9thode de d\u00e9termination"}}},"{\"value\":{\"entity-type\":\"item\",\"numeric-id\":13414952,\"id\":\"Q13414952\"},\"type\":\"wikibase-entityid\"}":{"text\/html":{"fr":{"P459":"SHA-1<\/a>"}},"text\/plain":{"fr":{"P459":"SHA-1"}}}}" class="wbmi-entityview-statementsGroup wbmi-entityview-statementsGroup-P4092 oo-ui-layout oo-ui-panelLayout oo-ui-panelLayout-framed">
b3292265ec1558c9724ae2715cda6897a313eadb
50 591 octet
900 pixel
900 pixel
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 | 5 août 2014 à 21:29 | 900 × 900 (49 kio) | Numéro 1963 | User created page with UploadWizard |
Utilisation du fichier
La page suivante utilise ce fichier :
Usage global du fichier
Les autres wikis suivants utilisent ce fichier :
- Utilisation sur bs.wikipedia.org
- Utilisation sur en.wikipedia.org
Ce document provient de « https://fr.wikipedia.org/wiki/Fichier:Triple_Jupiter_Eclipse.jpg ».