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HST WFC3 Jupiter Image (June 7, 2010) – Detail
About the Object
- DistanceDistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.The semi-major axis of Jupiter's orbit about the Sun is 5.2 astronomical units (483 million miles or 778 million km). On June 7, 2010 Jupiter was 475 million miles from Earth.
- DimensionsDimensionsThe physical size of the object or the apparent angle it subtends on the sky.The planet has a diameter of roughly 88,789 miles (142,984 km) at the equator.
About the Data
- Data DescriptionData DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.The image was created from Hubble data from proposal 12119: A. Simon-Miller (NASA Goddard Space Flight Center), H. Hammel (Space Science Institute, Boulder, Colo.), I. de Pater (University of California, Berkeley), L. Fletcher (University of Oxford), G. Orton (Jet Propulsion Laboratory), M. Wong (University of California, Berkley), A. Sanchez-Lavega (University of the Basque Country, Spain), J. Clarke (Boston University), and K. Noll (STScI). Note: The comparison data from HST WFC3 observations taken in 2009 are from proposals 12003 and 12045: 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). - InstrumentInstrumentThe science instrument used to produce the data.HST>WFC3/UVIS
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.June 7, 2010
- FiltersFiltersThe camera filters that were used in the science observations.F395N (395 nm), F502N (502 nm), and F631N (631 nm)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Jupiter
- Object DescriptionObject DescriptionThe type of astronomical object.Planet
- Release DateJune 16, 2010
- Science ReleaseMysterious Flash on Jupiter Left No Debris Cloud
- Credit
The 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: F395N (395 nm) Green: F502N (502 nm) Red: F631N (631 nm)
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov
