Archivo de imágenes de Hubble

Mapas globales de Júpiter del programa OPAL del Hubble

Scientists have produced new maps of Jupiter using the Wide Field Camera 3 on NASA's Hubble Space Telescope. Data for the two maps shown here were taken during Hubble Outer Planet Atmospheres Legacy program observations of Jupiter on Jan. 19, 2015, from 2:00 UT to 12:30 UT (upper...

Fecha
Jan 1, 2015
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2015-37-3638-image
Por

Scientists have produced new maps of Jupiter using the Wide Field Camera 3 on NASA's Hubble Space Telescope. Data for the two maps shown here were taken during Hubble Outer Planet Atmospheres Legacy program observations of Jupiter on Jan. 19, 2015, from 2:00 UT to 12:30 UT (upper panel) and from 15:00 UT to 23:40 UT (bottom panel). The movement of the clouds can be seen when comparing the two maps.

Credits

NASA, ESA, A. Simon (GSFC), M. Wong (UC Berkeley), and G. Orton (JPL-Caltech)

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 proposal : A. Simon (GSFC), M. Wong (UC Berkeley), and G. Orton (JPL-Caltech).
InstrumentHST>WFC3/UVIS
Exposure DatesJanuary 19, 2015
Filters395 nm, 502 nm, and 631 nm
About The Image
Color InfoThese images are a composite of separate exposures acquired by the WFC3 instrument on the Hubble Space Telescope. Several filters were used to sample narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F395N (395 nm) Green: F502N (502 nm) Red: F631N (631 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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