Myriad of Stars in Spiral Galaxy NGC 300

Stsci_2004-13e_1024

stsci_2004-13e April 8th, 2004

Credit: NASA, ESA, and The Hubble Heritage Team (AURA/STScI) Acknowledgment: F. Bresolin (Institute for Astronomy, U. Hawaii) and the Digitized Sky Survey

Myriads of stars embedded in the heart of the nearby galaxy NGC 300 can be singled out like grains of sand on a beach in this Hubble Space Telescope image. The Hubble telescope's exquisite resolution enables it to see the stars as individual points of light, despite the fact that the galaxy is millions of light-years away. NGC 300 is a spiral galaxy similar to our own Milky Way galaxy. It is a member of a nearby group of galaxies known as the Sculptor group, named for the southern constellation where the group can be found. The distance to NGC 300 is 6.5 million light-years, making it one of the Milky Way's closer neighbors. At this distance, only the brightest stars can be picked out from ground-based images. With a resolution some 10 times better than ground-based telescopes, Hubble's Advanced Camera for Surveys(ACS) resolves many more stars in this galaxy than can be detected from the ground. The color composite was made from filtered images taken in blue, green, and infrared light. Hot, young blue stars appear in clusters that form in the galaxy's spiral arms. Ribbons of deep red stars mark the location of gauzy curtains of dust that partially hide the light of the stars behind them. Near the center of the image is the bright and compact nucleus of the galaxy where even the ACS loses the ability to separate the densely packed stars. The individual exposures that were combined to make this new image were taken in July and September 2002. These Hubble data are being used to test a new method for measuring distances to galaxies and to compare it with the more traditional methods, such as the period-luminosity relationship of pulsating stars known as Cepheid variables. Measuring distances is a perpetual but important concern for astronomers. Some of the luminous blue specks in this image, young and massive stars called blue supergiants, are among the brightest stars seen in spiral galaxies like NGC 300. By combining the stellar brightness with

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2004/news-2004-13

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
NGC 300
Subject - Local Universe
Galaxy > Type > Spiral
Star

Distance Details Distance

Universescale2
6,500,000 light years
Stsci_2004-13e_128
 

Position Details Position Details

Position (ICRS)
RA = 0h 54m 39.4s
DEC = -37° 38’ 9.1”
Orientation
North is 171.7° CW
Field of View
3.0 x 4.7 arcminutes
Constellation
Sculptor

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (B) 435.0 nm
Green Hubble (ACS) Optical (V) 555.0 nm
Red Hubble (ACS) Optical (I) 814.0 nm
Spectrum_base
Blue
Green
Red
Stsci_2004-13e_1280
×
ID
2004-13e
Subject Category
C.5.1.1   C.3  
Subject Name
NGC 300
Credits
NASA, ESA, and The Hubble Heritage Team (AURA/STScI) Acknowledgment: F. Bresolin (Institute for Astronomy, U. Hawaii) and the Digitized Sky Survey
Release Date
2004-04-08T00:00:00
Lightyears
6,500,000
Redshift
6,500,000
Reference Url
https://hubblesite.org/contents/news-releases/2004/news-2004-13
Type
Observation
Image Quality
Good
Distance Notes
Distance in lightyears
Facility
Hubble, Hubble, Hubble
Instrument
ACS, ACS, ACS
Color Assignment
Blue, Green, Red
Band
Optical, Optical, Optical
Bandpass
B, V, I
Central Wavelength
435, 555, 814
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
13.66427171036, -37.63585831329
Reference Dimension
1186.00, 1869.00
Reference Pixel
-402.99101207909, -315.24499924733
Scale
-0.00004213352, 0.00004213352
Rotation
-171.66208108116
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center FITS X FITS Y EPO X EPO Y 571.47 1656.49 556.78 917.66 433.92 1737.22 825.80 705.33 505.30 1877.38 632.00 429.00 589.44 2063.39 398.78 61.96 831.10 1508.27 61.03 1293.25 655.75 1338.14 480.65 1600.11 422.62 1430.54 947.30 1336.23 438.30 1270.97 960.88 1677.95 Center Pixel Coordinates: 593.00 13.72594432977 934.50 -37.68236084867
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-p0413e-f-3557x5606.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0413e-f-3557x5606.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2004/13
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
6,500,000 light years

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