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Uranus and Neptune (Hubble)

The Hubble Space Telescope captured these images of the mysterious ice giants Uranus, left, and Neptune, right. Shortly after launch in 2021, the James Webb Space Telescope will unlock secrets of the atmospheres of both planets.
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. - InstrumentInstrumentThe science instrument used to produce the data.Left: ACS, Right: WFC3/UVIS
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.August 2005 and November 5-17, 2018
- FiltersFiltersThe camera filters that were used in the science observations.Left: Clear, F330W, F475W, F606W, F814W Right: F467M, F547M, F657N, F763M, F845M
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Uranus and Neptune
- Object DescriptionObject DescriptionThe type of astronomical object.Gas giants with storm clouds
- Release DateFebruary 26, 2020
- Science ReleaseExamining Ice Giants with NASA’s Webb Telescope
- CreditImage: NASA, ESA, Mark Showalter (SETI Institute), Amy Simon (NASA-GSFC), Michael Wong (UC Berkeley), Andrew Hsu (UC Berkeley)

These images are a composite of separate exposures acquired by the WFC3 and ACS instruments on the Hubble Space Telescope. Several filters were used to sample specific 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: Uranus: Blue: F330W Green: F475W Orange: F606W Red: F814W Neptune: Blue: F467M Green: F547M Yellow: F657N Orange: F763M Red: F845M
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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov
NASA, ESA, Mark Showalter (SETI Institute), Amy Simon (NASA-GSFC), Michael Wong (UC Berkeley), Andrew Hsu (UC Berkeley)









