Hubble image archive

Westerlund 2: Detail 4

The red dots scattered throughout the landscape around Westerlund 2 are a rich population of newly forming stars still wrapped in their gas-and-dust cocoons. These tiny, faint stars are between 1 million and 2 million years old and have not yet ignited the hydrogen in their cores...

Date
Jan 1, 2015
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2015-12-3522-image
By

The red dots scattered throughout the landscape around Westerlund 2 are a rich population of newly forming stars still wrapped in their gas-and-dust cocoons. These tiny, faint stars are between 1 million and 2 million years old and have not yet ignited the hydrogen in their cores. Hubble's near-infrared vision allows astronomers to identify these fledgling stars.

Credits

NASA, ESA, the Hubble Heritage Team (STScI/AURA), A. Nota (ESA/STScI), and the Westerlund 2 Science Team

Image Details

About The Object
Object NameWesterlund 2, Gum 29
Object DescriptionCluster and Starforming Region
R.A. Position10h 23m 58.1s
Dec. Position-57° 45' 48.96"
ConstellationCarina
Distance20,000 light-years (6,130 parsecs)
About The Data
Data DescriptionData of Westerlund 2 were obtained from the HST proposals : A. Nota (ESA/STScI), E. Sabbi and C. Christian (STScI), E. Grebel and P. Zeidler (Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg), M. Tosi (INAF, Osservatorio Astronomico di Bologna), A. Bonanos (National Observatory of Athens, Astronomical Institute), and S. de Mink (University of Amsterdam); and : Z. Levay, M. Mutchler, J. Mack, L. Frattare, S. Meyett, M. Livio, and C. Christian (STScI/AURA), K. Noll (NASA/GSFC), A. Nota (STScI/ESA), and E. Sabbi (STScI).
InstrumentHST>ACS/WFC and HST>WFC3/IR
Exposure DatesSeptember 2013 - November 2014, Total Exposure Time: 23,074 seconds
FiltersACS/WFC: F555W (V) and F814W (I) WFC3/IR: F125W (J)
About The Image
Color InfoThese images are composites of separate exposures acquired by the ACS and the WFC3 instruments on the Hubble Space Telescope. Several filters were used to sample broad and narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F555W (V) Green: F555W (V) and F814W (I) Red: F814W (I)

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