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Supernova Remnant LMC N132D
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.05h 25m 1.4s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.-69° 38' 31.0"
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Dorado
- 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.170,000 light-years (52,000 parsecs)
- DimensionsDimensionsThe physical size of the object or the apparent angle it subtends on the sky.This image is 3 arcminutes (150 light-years or 46 parsecs) wide.
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 Hubble images/spectrum were created from data from proposal 11503: K. Noll (STScI) and J. Green, C. Froning, and K. France (University of Colorado, Boulder); and proposal 12001: J. Green (University of Colorado, Boulder). Acknowledgments for N132D Observers: K. Noll (STScI) and J. Green, C. Froning, and K. France (University of Colorado, Boulder) Data Analysis: J. Anderson and M. Mutchler (STScI), and C. Froning and J. Green (University of Colorado, Boulder) Image Composition: Z. Levay and L. Frattare (STScI) Text: L. Frattare, D. Weaver, and R. Villard (STScI) Illustrations: A. Feild and Z. Levay (STScI) Video Animation: G. Bacon (STScI) Science Consultants: M. Livio (STScI) and C. Froning and J. Green (University of Colorado, Boulder) - InstrumentInstrumentThe science instrument used to produce the data.HST>ACS/WFC and HST>WFC3/UVIS
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.January 21-22, 2004 (ACS) and August 2, 2009 (WFC3)
- FiltersFiltersThe camera filters that were used in the science observations.ACS: F673N WFC3: F475W (g), F550M (y) F658N (H-alpha + [N II]), and F850LP (z)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.LMC N132D, SNR J052501-693842
- Object DescriptionObject DescriptionThe type of astronomical object.Supernova Remnant
- Release DateSeptember 9, 2009
- Science ReleaseHubble Opens New Eyes on the Universe
- Credits
The image is a composite of separate exposures made by the WFC3 and ACS instruments on the Hubble Space Telescope. Five filters were used to sample broad and narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Pink: F850LP (z) Orange: F658N (H-alpha + [N II]) White: F673N ([S II]) Green: F550M (y) Blue: F475W (g)
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Details
Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, MD
claire.andreoli@nasa.gov
