Archivo de imágenes de Hubble

Hubble interactuando con la galaxia Mrk 273

Markarian 273 is a galaxy with a bizarre structure that somewhat resembles a toothbrush. The Hubble image shows an intricate central region and a striking tail that extends diagonally towards the bottom-right of the image. The tail is about 130 thousand light-years long and is st...

Fecha
Jan 1, 2008
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2008-16-2307-image
Por

Markarian 273 is a galaxy with a bizarre structure that somewhat resembles a toothbrush. The Hubble image shows an intricate central region and a striking tail that extends diagonally towards the bottom-right of the image. The tail is about 130 thousand light-years long and is strongly indicative of a merger between two galaxies. Markarian 273 has an intense region of starburst, where 60 solar masses of new stars are born each year. Near-infrared observations reveal a nucleus with two components. Markarian 273 is one of the most luminous galaxies when observed in the infrared, and is located 500 million light-years away from Earth.

This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the occasion of its 18th anniversary on 24th April 2008.

Credits

NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)

Detalles de la imagen

About The Object
Object NameMrk 273, UGC 8696, I Zw 071
Object DescriptionInteracting Galaxies
R.A. Position13h 44m 42.28s
Dec. Position55° 53' 10.5"
ConstellationUrsa Major
Distance500 million light-years (150 million parsecs)
About The Data
Data DescriptionHST Proposal: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
InstrumentHST>ACS/WFC
Exposure DatesNovember 16, 2001, Exposure Time: 37 minutes
FiltersF435W (B) and F814W (I)

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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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