Hubble image archive

Trio of Images of the Arches Cluster

These images of the Arches cluster, taken by three different telescopes, reveal progressively more detail in the tightly packed collection of about 2,000 stars. The Arches is the densest star cluster in our Milky Way Galaxy and resides in our galaxy's crowded core.Astronomers use...

Date
Jan 1, 2005
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2005-05-1652-image
By

These images of the Arches cluster, taken by three different telescopes, reveal progressively more detail in the tightly packed collection of about 2,000 stars. The Arches is the densest star cluster in our Milky Way Galaxy and resides in our galaxy's crowded core.

Astronomers used the image at right, taken with Hubble's Near Infrared Camera and Multi-Object Spectrometer, to determine if stars in the cluster have a weight limit at birth. Hubble's infrared camera is well suited to analyze the cluster because it penetrates the dusty core of our galaxy and produces sharp images, allowing the telescope to see individual stars in a tightly packed grouping.

Credits

Left: NASA, ESA, D. Figer (STScI);
Middle: G. Serabyn (JPL), D. Shupe (Caltech) and D. Figer (STScI)
Right: NASA, ESA and D. Figer (STScI)

Image Details

About The Object
Object NameArches Cluster
Object DescriptionStar Cluster
R.A. Position17h 45m 50.5s
Dec. Position-28° 49' 27.99"
ConstellationSagittarius
Distance25,000 light-years away (8,000 parsecs)
About The Data
Data DescriptionThese data are from the HST program : D. Figer (STScI)
InstrumentLick>3m (left), Keck I>10m ( right), HST>NICMOS (right)
Exposure Dates1994 (Lick, left), 1996 (Keck, right), September 13-14, 1997, Exposure Time: 1.2 hours (HST, right)

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Source

Image and source material are credited to the official mission archive linked below.

View on NASA.gov

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