Archivo de imágenes de Hubble

Júpiter, Hubble WFC3: 8 de agosto de 2009

CreditsNASA, ESA, M. Wong (University of California, Berkeley), H.B. Hammel (Space Science Institute, Boulder, Colo.), I. de Pater (University of California, Berkeley), and the Jupiter Impact Team

Fecha
Jan 1, 2010
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2010-16-2728-image
Por

Credits

NASA, ESA, M. Wong (University of California, Berkeley), H.B. Hammel (Space Science Institute, Boulder, Colo.), I. de Pater (University of California, Berkeley), and the Jupiter Impact Team

Detalles de la imagen

About The Object
Object NameJupiter
Object DescriptionPlanet
DistanceThe semi-major axis of Jupiter's orbit about the Sun is 5.2 astronomical units (483 million miles or 778 million km).
DimensionsThe planet has a diameter of roughly 88,789 miles (142,984 km) at the equator.
About The Data
Data DescriptionThe image was created from Hubble data from proposals and : H. Hammel (Space Science Institute, Boulder, Colo.), A. Simon-Miller (NASA Goddard Space Flight Center), J. Clarke (Boston University), I. de Pater (University of California, Berkeley), K. Noll (STScI), G. Orton (Jet Propulsion Laboratory), A. Sanchez-Lavega (University of the Basque Country, Spain), and M. Wong (University of California, Berkley); and proposal : I. de Pater, P. Marcus, X. Asay-Davis, and M. Wong (University of California, Berkeley), and C. Go (University of San Carlos).
InstrumentHST>WFC3/UVIS
Exposure DatesAugust 8, 2009
FiltersFQ437N (437 nm), Q508N (508nm), and FQ634N (634 nm)
About The Image
Color InfoThe image is a composite of separate exposures made by the WFC3 instrument on the Hubble Space Telescope. Three filters were used to sample narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: FQ437N (437 nm) Green: Q508N (508nm) Red: FQ634N (634 nm)

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Fuente

La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.

Ver en NASA.gov

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