Ta'ãnga:PIA07712_-_F_ring_animation.gif
From Wikipedia, the free encyclopedia
PIA07712_-_F_ring_animation.gif (450 × 450 píxeles; tamaño de archivo: 3,43 MB; tipo MIME: image/gif, bucleado, 65 frames, 26s)
Ko marandurenda haꞌehína Wikimedia Commons guive ha ikatu ojeipuru ambue tembiaporãme. Pe ñemombeꞌupy oĩva marandurenda ñemombeꞌupy kuatia ryepýpe ojehechauka koꞌápe.
Resumen
Mombe'uangaPIA07712 - F ring animation.gif |
This movie sequence from Cassini shows dark drapes in the inner strands of the F ring caused by the gravitational influence of the shepherd moon Prometheus (102 kilometers, 63 miles across). Prometheus appears first in the sequence, interior to the F ring, and Pandora (84 kilometers, 52 miles across) follows along outside of the ring. Radial structure in the bright core of the ring is visible throughout the movie. Prometheus orbits closer to Saturn, and thus faster, than the icy particles that make up the F ring. The moon passes comes closest to the ring at “apoapse”, when it is farthest from Saturn. It is during these apoapse passages that Prometheus has its greatest influence on the fine ring material. With time, the ring material previously affected falls behind so that on the next apoapse passage of Prometheus, a new gore in the inner ring material is made. The material closer to Prometheus orbits the planet faster than the material closer to the bright F ring core. The gores, together with the sheared-out material due to differential orbital motion, create the dark, diagonal drapes. Several background stars are seen moving across the field during the movie. The visible light images in this sequence were acquired using the narrow angle camera on April 13, 2005 from a distance of approximately 1.2 million kilometers (700,000 miles) from Saturn. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org. This is a truncation of NASA's half-size animated gif version of the sequence. The full size image sequence is also available at http://photojournal.jpl.nasa.gov/animation/PIA07712. |
Arange | |
Moõgui oguenohẽ | http://ciclops.org/view.php?id=1361 |
Apohára | NASA/JPL/Space Science Institute |
Otras versiones |
|
![]() |
Este archivo fue catalogado por Jet Propulsion Lab de la Administración Nacional de Aeronáutica y del Espacio (NASA) de los Estados Unidos de Américabajo el identificador de foto: PIA07712.Esta etiqueta no indica el estado de los derechos de autor del trabajo adjunto. Se requiere una etiqueta de derechos de autor normal. Para más información vea Commons:Sobre las licencias. Otros idiomas:
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 ∙ +/− |
Derivative works of this file:
- PIA07712 - F ring animation framerate 1.ogv
- PIA07712 - F ring animation.ogv
- PIA07712 - F ring animation framerate 5.ogv
Licencia
Public domainPublic domainfalsefalse |
![]() |
Este archivo es de dominio público porque fue creado por la NASA. Las políticas sobre copyright de la NASA estipulan que «el material de la NASA no está protegido con copyright a menos que se indique lo contrario». (Políticas sobre copyright de la NASA o Políticas sobre la utilización de imágenes del Jet Propulsion Laboratory). | ![]() |
![]() |
Advertencias:
|
Leyendas
Elementos representados en este archivo
representa a español
13 jasyrundy 2005
tipo de archivo español
image/gif
Marandurenda rembiasakue
Ejopy peteĩ ára/aravo rehe rehecha hag̃ua pe marandurenda ojehechaukaháicha upe jave.
Ára/Aravo | Michĩháicha | Tuichakue | Puruhára | Jehaimombyky | |
---|---|---|---|---|---|
ko’ag̃agua | 19:51 24 jasypateĩ 2007 | ![]() | 450 × 450 (3,43 MB) | WolfmanSF | Reduce file size by deleting alternate frames. Double delay setting to maintain speed of animation. |
09:48 23 jasypateĩ 2007 | ![]() | 450 × 450 (6,44 MB) | WolfmanSF | truncate down to 122 frames | |
02:00 23 jasypateĩ 2007 | ![]() | 450 × 450 (6,91 MB) | WolfmanSF | further truncation down to 131 frames | |
09:02 22 jasypateĩ 2007 | ![]() | 450 × 450 (7,12 MB) | WolfmanSF | ||
10:01 21 jasypateĩ 2007 | ![]() | 450 × 450 (9,01 MB) | WolfmanSF | {{Information |Description=This movie sequence from Cassini shows dark drapes in the inner strands of the F ring caused by the gravitational influence of the shepherd moon Prometheus (102 kilometers, 63 miles across). Prometheus appears first in the sequ |
Marandurenda jeporu
La siguiente página usa este archivo:
Marandurenda jepuru opaite tembiapópe
Ko'ã ambue wiki oipuru ko marandurenda:
- Jeporu af.wikipedia.org rehe
- Jeporu ar.wikipedia.org rehe
- Jeporu be.wikipedia.org rehe
- Jeporu bn.wikipedia.org rehe
- Jeporu cs.wikipedia.org rehe
- Jeporu de.wikipedia.org rehe
- Jeporu en.wikipedia.org rehe
- Jeporu eo.wikipedia.org rehe
- Jeporu fa.wikipedia.org rehe
- Jeporu fr.wikipedia.org rehe
- Jeporu gl.wikipedia.org rehe
- Jeporu he.wikipedia.org rehe
- Jeporu hy.wikipedia.org rehe
- Jeporu id.wikipedia.org rehe
- Jeporu it.wikipedia.org rehe
- Jeporu lb.wikipedia.org rehe
- Jeporu mk.wikipedia.org rehe
- Jeporu pt.wikipedia.org rehe
- Jeporu ro.wikipedia.org rehe
- Jeporu ru.wikipedia.org rehe
- Jeporu sk.wikipedia.org rehe
- Jeporu tr.wikipedia.org rehe
- Jeporu uk.wikipedia.org rehe
- Jeporu zh-classical.wikipedia.org rehe
- Jeporu zh.wikipedia.org rehe