Hubble Makes the First Precise Distance Measurement to an Ancient Globular Star Cluster

Stsci_2018-24b_1024

stsci_2018-24b April 4th, 2018

Credit: NASA, ESA, and T. Brown and S. Casertano (STScI) Acknowledgement: NASA, ESA, and J. Anderson (STScI)

Refined stellar yardstick helps astronomers improve stellar evolution models

When you want to know the size of a room, you use a measuring tape to calculate its dimensions.

But you can’t use a tape measure to cover the inconceivably vast distances in space. And, until now, astronomers did not have an equally precise method to accurately measure distances to some of the oldest objects in our universe – ancient swarms of stars outside the disk of our galaxy called globular clusters.

Estimated distances to our Milky Way galaxy’s globular clusters were achieved by comparing the brightness and colors of stars to theoretical models and observations of local stars. But the accuracy of these estimates varies, with uncertainties hovering between 10 percent and 20 percent.

Using NASA’s Hubble Space Telescope, astronomers were able to use the same sort of trigonometry that surveyors use to precisely measure the distance to NGC 6397, one of the closest globular clusters to Earth. The only difference is that the angles measured in Hubble’s camera are infinitesimal by earthly surveyors’ standards.

The new measurement sets the cluster’s distance at 7,800 light-years away, with just a 3 percent margin of error, and provides an independent estimate for the age of the universe. The Hubble astronomers calculated NGC 6397 is 13.4 billion years old and so formed not long after the big bang. The new measurement also will help astronomers improve models of stellar evolution.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2018/news-2018-24

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
NGC 6397
Subject - Milky Way
Star > Grouping > Cluster > Globular

Distance Details Distance

Universescale1
9,000 light years
Stsci_2018-24b_128
 

Position Details Position Details

Position (ICRS)
RA = 17h 40m 40.1s
DEC = -53° 40’ 11.7”
Orientation
North is 0.1° CCW
Field of View
3.3 x 2.5 arcminutes
Constellation
Ara

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Cyan Hubble (ACS/WFC) Optical (B) 435.0 nm
Orange Hubble (ACS/WFC) Optical (V) 625.0 nm
Spectrum_base
Cyan
Orange
Stsci_2018-24b_1280
×
ID
2018-24b
Subject Category
B.3.6.4.2  
Subject Name
NGC 6397
Credits
NASA, ESA, and T. Brown and S. Casertano (STScI) Acknowledgement: NASA, ESA, and J. Anderson (STScI)
Release Date
2018-04-04T00:00:00
Lightyears
9,000
Redshift
9,000
Reference Url
https://hubblesite.org/contents/news-releases/2018/news-2018-24
Type
Observation
Image Quality
Good
Distance Notes
Facility
Hubble, Hubble
Instrument
ACS/WFC, ACS/WFC
Color Assignment
Cyan, Orange
Band
Optical, Optical
Bandpass
B, V
Central Wavelength
435, 625
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
265.16703836449, -53.66992797621
Reference Dimension
2462.00, 1847.00
Reference Pixel
1427.45804808755, 1039.71204885490
Scale
-0.00002225409, 0.00002225409
Rotation
0.12661082060
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
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-p1824b-f-4924x3693.tif
Metadata Date
2018-04-02T17:46:39-04:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

×
Universescalefull
9,000 light years

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