The Antennae Galaxies/NGC 4038-4039

Stsci_2006-46a_1024

stsci_2006-46a October 16th, 2006

Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)- ESA/Hubble Collaboration Acknowledgment: B. Whitmore (Space Telescope Science Institute)

This new NASA Hubble Space Telescope image of the Antennae galaxies is the sharpest yet of this merging pair of galaxies. During the course of the collision, billions of stars will be formed. The brightest and most compact of these star birth regions are called super star clusters. The two spiral galaxies started to interact a few hundred million years ago, making the Antennae galaxies one of the nearest and youngest examples of a pair of colliding galaxies. Nearly half of the faint objects in the Antennae image are young clusters containing tens of thousands of stars. The orange blobs to the left and right of image center are the two cores of the original galaxies and consist mainly of old stars criss-crossed by filaments of dust, which appears brown in the image. The two galaxies are dotted with brilliant blue star-forming regions surrounded by glowing hydrogen gas, appearing in the image in pink. The new image allows astronomers to better distinguish between the stars and super star clusters created in the collision of two spiral galaxies. By age dating the clusters in the image, astronomers find that only about 10 percent of the newly formed super star clusters in the Antennae will survive beyond the first 10 million years. The vast majority of the super star clusters formed during this interaction will disperse, with the individual stars becoming part of the smooth background of the galaxy. It is however believed that about a hundred of the most massive clusters will survive to form regular globular clusters, similar to the globular clusters found in our own Milky Way galaxy. The Antennae galaxies take their name from the long antenna-like "arms" extending far out from the nuclei of the two galaxies, best seen by ground-based telescopes. These "tidal tails" were formed during the initial encounter of the galaxies some 200 to 300 million years ago. They give us a preview of what may happen when our Milky Way galaxy will collide with the neighboring Andromeda galaxy in several billion years.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2006/news-2006-46

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

Image Details Image Details

Image Type
Observation
Object Name
NGC 4038/4039 Antennae Galaxy
Subject - Local Universe
Galaxy > Type > Interacting
Galaxy > Grouping > Multiple

Distance Details Distance

Universescale2
62,000,000 light years
Stsci_2006-46a_128
 

Position Details Position Details

Position (FK5)
RA = 12h 1m 54.0s
DEC = -18° 53’ 48.8”
Orientation
North is 149.2° CCW
Field of View
-3.3 x -3.3 arcminutes
Constellation
Corvus

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (B) 435.0 nm
Green Hubble (ACS) Optical (y) 550.0 nm
Magenta Hubble (ACS) Optical (Halpha [N II]) 658.0 nm
Red Hubble (ACS) Optical (I) 814.0 nm
July 21, 2004 and February 16, 2005
Spectrum_base
Blue
Green
Magenta
Red
Stsci_2006-46a_1280
×
ID
2006-46a
Subject Category
C.5.1.7   C.5.5.2  
Subject Name
NGC 4038/4039, Antennae Galaxy
Credits
NASA, ESA, and the Hubble Heritage Team (STScI/AURA)- ESA/Hubble Collaboration Acknowledgment: B. Whitmore (Space Telescope Science Institute)
Release Date
2006-10-16T00:00:00
Lightyears
62,000,000
Redshift
62,000,000
Reference Url
https://hubblesite.org/contents/news-releases/2006/news-2006-46
Type
Observation
Image Quality
Good
Distance Notes
62 million light-years (19 Megaparsecs)
Facility
Hubble, Hubble, Hubble, Hubble
Instrument
ACS, ACS, ACS, ACS
Color Assignment
Blue, Green, Magenta, Red
Band
Optical, Optical, Optical, Optical
Bandpass
B, y, Halpha [N II], I
Central Wavelength
435, 550, 658, 814
Start Time
2004-07-21T00:00:00, 2004-07-21T00:00:00, 2004-07-21T00:00:00, 2004-07-21T00:00:00
Integration Time
Dataset ID
Notes
J
Coordinate Frame
FK5
Equinox
2000.0
Reference Value
180.4750814870000113, -18.8968899750000006
Reference Dimension
3915.0000000000000000, 3885.0000000000000000
Reference Pixel
1113.5480041499999970, 1098.6982421899999736
Scale
0.0000139449542538, -0.0000139449542538
Rotation
149.1509604261781590
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p0646a-f-3915x3885.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0646a-f-3915x3885.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2006/46
Metadata Date
2022-07-06T00:00:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

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Universescalefull
62,000,000 light years

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