Hubble Probes the Archeology of Our Milky Way's Ancient Hub

Stsci_2018-01b_1024

stsci_2018-01b January 11th, 2018

Credit: Image: NASA, ESA, and T. Brown (STScI) Science: NASA, ESA, W. Clarkson (University of Michigan-Dearborn), and A. Calamida and K. Sahu (STScI)

Every star has a story to tell. Study a star and it will give you information about its composition, age and possibly even clues to where it first formed. The stars residing in the oldest structure of our Milky Way galaxy, the central bulge, offer insight into how our pinwheel-shaped island of myriad stars evolved over billions of years. Think of our Milky Way as a pancake-shaped structure with a big round dollop of butter in the middle — that would be our galaxy’s central hub.

For many years, astronomers had a simple view of our Milky Way’s bulge as a quiescent place composed of old stars, the earliest homesteaders of our galaxy. A new analysis of about 10,000 normal sun-like stars in the bulge reveals that our galaxy’s hub is a dynamic environment of various ages zipping around at different speeds, like travelers bustling about a busy airport. This conclusion is based on nine years’ worth of archival data from the Hubble Space Telescope. The faster-moving and later-generation stars may have arrived at the hub through our Milky Way cannibalizing smaller galaxies. They mingle with a different population of older, slowing-moving stars. Currently, only Hubble has sharp enough resolution to simultaneously measure the motions of thousands of sun-like stars at the distance of the galaxy’s bulge.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2018/news-2018-01

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
BTS SWEEPS
Subject - Milky Way
Galaxy > Component > Bulge

Distance Details Distance

Universescale1
26,000 light years
Stsci_2018-01b_128
 

Position Details Position Details

Position (ICRS)
RA = 17h 58m 58.0s
DEC = -29° 12’ 20.6”
Orientation
North is 16.9° CCW
Field of View
2.2 x 1.9 arcminutes
Constellation
Sagittarius

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (WFC3) Optical (V) 505.0 nm
Green Hubble (WFC3) Optical (I) 814.0 nm
Red Hubble (WFC3) Infrared (YJ) 1.1 µm
Red Hubble (WFC3) Infrared (H) 1.6 µm
Spectrum_base
Blue
Green
Red
Red
Stsci_2018-01b_1280
×
ID
2018-01b
Subject Category
B.5.4.1  
Subject Name
BTS SWEEPS
Credits
Image: NASA, ESA, and T. Brown (STScI) Science: NASA, ESA, W. Clarkson (University of Michigan-Dearborn), and A. Calamida and K. Sahu (STScI)
Release Date
2018-01-11T00:00:00
Lightyears
26,000
Redshift
26,000
Reference Url
https://hubblesite.org/contents/news-releases/2018/news-2018-01
Type
Observation
Image Quality
Good
Distance Notes
Facility
Hubble, Hubble, Hubble, Hubble
Instrument
WFC3, WFC3, WFC3, WFC3, WFC3
Color Assignment
Blue, Green, Red, Red
Band
Optical, Optical, Infrared, Infrared
Bandpass
V, I, YJ, H
Central Wavelength
505, 814, 1100, 1600
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
269.74186674792, -29.20572694872
Reference Dimension
3336.00, 2823.00
Reference Pixel
1664.57744102722, 822.24085422810
Scale
-0.00001098746, 0.00001098746
Rotation
16.91692105717
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-p1801b-f-3336x2823.tif
Metadata Date
2018-01-05T16:54:10-05:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

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Universescalefull
26,000 light years

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