COS Spectrum of Supernova Remnant LMC N132D

 COS Spectrum of Supernova Remnant LMC N132D

Spectrum of the supernova remnant LMC N132D taken with Hubble's Cosmic Origins Spectrograph.

Credits

NASA, ESA, and the Hubble SM4 ERO Team

About The Object
Object Name LMC N132D, SNR J052501-693842
Object Description Supernova Remnant
Constellation Dorado
Distance 170,000 light-years (52,000 parsecs)
About The Data
Data Description The Hubble images/spectrum were created from data from proposal : K. Noll (STScI) and J. Green, C. Froning, and K. France (University of Colorado, Boulder); and proposal : 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)
Instrument HST>COS/FUV and HST>COS/NUV
Exposure Dates August 10, 2009
Filters G130M (130nm) and G160M (160 nm)
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The 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.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: 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.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.