News Release Archive:

News Release 16 of 47

August 16, 2012 10:00 AM (EDT)

News Release Number: STScI-2012-35

Hubble Watches Star Clusters on a Collision Course

Technical facts about this news release:

About the Object
Object Name: 30 Doradus
Object Description: Nebula in the Large Magellanic Cloud
Position (J2000): R.A. 05h 38m 42s
Dec. -69° 06' 03''
Constellation: Dorado
Distance: 170,000 light-years (52,000 parsecs)
About the Data
Data Description:

The members of the science team are: E. Sabbi and D.J. Lennon (ESA/STScI), M. Gieles (University of Cambridge, UK), S.E. de Mink (STScI/JHU), N.R. Walborn, J. Anderson, A. Bellini, N. Panagia, and R. van der Marel (STScI), and J. Maíz Apellániz (Instituto de Astrofísica de Andalucía, CISC, Spain)

The image was created from Hubble data from proposal 11360: R. O'Connell (University of Virginia), B. Balick (University of Washington), H. Bond (STScI), D. Calzetti (University of Massachusetts), M. Carollo (Swiss Federal Institute of Technology, Zurich), M. Disney (University of Wales, College of Cardiff), M. Dopita (Australian National University), J. Frogel (Ohio State University Research Foundation), D. Hall (University of Hawaii), J. Holtzman (New Mexico State University), P. McCarthy (Carnegie Institution of Washington), F. Paresce (European Southern Observatory, Germany), A. Saha (NOAO/AURA), J. Silk (University of Oxford), A. Walker (NOAO/CTIO), B. Whitmore (STScI), R. Windhorst (Arizona State University), and E. Young (University of Arizona).

Instrument: WFC3/UVIS WFC/IR
Exposure Date(s): October 20 - 27, 2009 October 20 - 27, 2009
Exposure Time: 11.7 hours 2.6 hours
Filters: F336W (U), F438W (B), F555W (V), F814W (I), and F656N (H-alpha)
About the Release
Credit: NASA, ESA, E. Sabbi (ESA/STScI)

Acknowledgment: R. O'Connell (University of Virginia, Charlottesville) and the WFC3 Science Oversight Committee
Release Date: August 16, 2012
Color: The images are composites of separate exposures made by the WFC3 instrument on the Hubble Space Telescope. Five filters were used to sample broad and narrow wavelength ranges for the UVIS image. The colors result from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are:
WFC3/UVIS image of 30 Dor
F336W (U) and F438W (B) blue
F555W (V) green
F814W (I) red
F656N (H-alpha) orange/red
Orientation: Compass and Scale Image of Merging Star Clusters in 30 Doradus