Hubble image archive

Hubble ACS Image of IC 4662

CreditsNASA, ESA, and K. McQuinn (University of Minnesota, Minneapolis)

Date
Jan 1, 2009
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2009-19-2560-image
By

Credits

NASA, ESA, and K. McQuinn (University of Minnesota, Minneapolis)

Image Details

About The Object
Object NameIC 4662
Object DescriptionStarburst Galaxy
R.A. Position17h 47m 8.86s
Dec. Position-64° 38' 30.33"
ConstellationPavo
Distance8 million light-years or 2.4 megaparsecs
Dimensions83 arcseconds (3,100 light-years or 960 parsecs) wide
About The Data
Data DescriptionThe image was created from Hubble data from proposal : I. Karachentsev (Russian Academy of Sciences, Special Astrophysical Observatory), B. Tully (University of Hawaii), V. Karachentseva (Kyiv University), A. Dolphin (Raytheon Company), S. Sakai (University of California, Los Angeles), E. Shaya (University of Maryland), and M. Sharina, L. Makarova, and D. Makarov (Russian Academy of Sciences, Special Astrophysical Observatory). The science team comprises: K. McQuinn and E. Skillman (University of Minnesota, Minneapolis), J. Cannon (Macalester College, MN), J. Dalcanton (University of Washington, Seattle), A. Dolphin (Raytheon Company), and D. Stark and D. Weisz (University of Minnesota, Minneapolis).
InstrumentHST>ACS
Exposure DatesMarch 28, 2004, Exposure Time: 35 minutes
FiltersF606W (R) and F814W (I)
About The Image
Color InfoThese images are composites of several separate exposures made by the ACS instrument on the Hubble Space Telescope. Two filters were used to sample broad wavelength ranges for each image. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are orange/yellow for the I-band (F814W) and cyan/blue for the wide V-band (F606W) filter. The images have been further adjusted so the colors more closely resemble their true visual appearance, particularly the red hydrogen emission of the star-forming regions. Cyan: F606W (R) Yellow: F814W (I)

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