ULLYSES Targets in LMC

Stsci_2020-50a_1024

stsci_2020-50a November 5th, 2020

Credit: NASA, ESA, STScI, R. Gendler

The universe would be a pretty boring place without stars. Without them, the universe would remain a diffuse plasma of mostly hydrogen and helium from the big bang. As the basic building blocks of the cosmos, stellar nuclear fusion furnaces forge new heavy elements, enriching their parent galaxy. The radiant energy from stars potentially nurtures the emergence of life on the most favorably located planets, as it did on Earth. To better understand stellar evolution, the Space Telescope Science Institute (STScI) in Baltimore, Maryland, has launched an ambitious new initiative with Hubble called ULLYSES (UV Legacy Library of Young Stars as Essential Standards). This is the largest observing program ever undertaken by NASA’s Hubble Space Telescope, which will be used to look at over 300 stars. Ultraviolet (UV) light from the target stars will be used to produce a library of the spectral fingerprints of young, low-mass stars from eight star-forming regions in the Milky Way, as well as fully mature high-mass stars in several nearby dwarf galaxies including the Magellanic Clouds. “One of the key goals of ULLYSES is to form a complete reference sample that can be used to create spectral libraries capturing the diversity of stars, ensuring a legacy dataset for a wide range of astrophysical topics. ULLYSES will have a lasting impact on future research by astronomers around the world,” said program lead Julia Roman-Duval of STScI. The Institute is now releasing the first set of ULLYSES observations to the astronomical community. These early targets are hot, massive, blue stars in several nearby dwarf galaxies. Hubble is located above Earth’s atmosphere, which filters out most UV radiation from space before it reaches ground-based telescopes. Hubble’s ultraviolet sensitivity makes it the only observatory optimized for the task because young stars radiate a lot of their energy in the UV as they grow chaotically in fits and starts while feeding on infalling gas and dust. ULLYSES will give astronomers a much better understanding of the birth of stars and how this relates to everything from planets to the formation and evolution of galaxies. Astronomers also want to learn how young low-mass stars affect the evolution and composition of planets around them. Intense UV radiation pulls apart molecules and penetrates circumstellar disks, where planets form, influencing their chemistry and affecting how long the disks survive. This has a direct bearing on planet habitability, atmospheric escape, and chemistry. “This unique collection will enable diverse and exciting astrophysical research across many fields,” Roman-Duval said. In addition, the torrential outflows from fully mature stars that are much more massive than our Sun shape their environments in dramatic ways. By targeting massive stars in nearby galaxies with low abundances in heavy elements, similar to the primitive composition of early galaxies, astronomers can gain insights into how their outflows may have influenced early galaxy evolution billions of years ago. The design and targets of these observations were selected in partnership with the astronomical community, allowing researchers from around the world to help develop the final program as well as have the opportunity to organize coordinated observations by other space- and ground-based telescopes at different wavelengths of light. STScI scientific and technical staff are designing software specifically related to the development of databases and web interfaces to ensure wide access to the library by the astronomical community. Tools for high-level science products and spectroscopic analysis are being developed. All of the data will be stored in STScI’s Mikulski Archive for Space Telescopes. The ULLYSES program will build a legacy for the future, creating a comprehensive database that astronomers will use for research for decades to come. The archive will also complement the portions of the star-formation story obtained with infrared-light observations from NASA’s upcoming James Webb Space Telescope. Working together, both Hubble and Webb will provide a holistic view of stars and the star-formation history of universe.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2020/news-2020-50

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
LMC Large Magellanic Cloud
Subject - Local Universe
Galaxy > Type > Irregular
Star > Evolutionary Stage > Young Stellar Object

Distance Details Distance

Universescale2
168,000 light years
Stsci_2020-50a_128
 

Position Details Position Details

Position (ICRS)
RA = 5h 11m 17.7s
DEC = -69° 56’ 46.5”
Orientation
North is 86.6° CCW
Field of View
9.6 x 7.9 degrees
Constellation
Mensa

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Red Ground-based image (FSQ106 STL11000) Optical (B) -
Stsci_2020-50a_1280
×
ID
2020-50a
Subject Category
C.5.1.6   C.3.1.2  
Subject Name
LMC, Large Magellanic Cloud
Credits
NASA, ESA, STScI, R. Gendler
Release Date
2020-11-05T00:00:00
Lightyears
168,000
Redshift
168,000
Reference Url
https://hubblesite.org/contents/news-releases/2020/news-2020-50
Type
Observation
Image Quality
Good
Distance Notes
Distance in Lightyears
Facility
Ground-based image
Instrument
FSQ106 STL11000
Color Assignment
Red, Green, Blue
Band
Optical, Optical, Optical
Bandpass
B, V, R
Central Wavelength
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
77.82368576192, -69.94624607775
Reference Dimension
4000.00, 3284.00
Reference Pixel
2471.89822606923, 2011.43111438285
Scale
-0.00239710161, 0.00239710161
Rotation
86.62362771121
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 170.30 718.74 1983.15 2380.43 166.82 755.19 2029.31 2387.50 208.88 786.07 2072.19 2334.78 129.30 782.51 2061.67 2437.64 184.88 865.56 2172.45 2371.33 70.92 845.03 2138.87 2516.81 127.02 881.03 2188.58 2446.52 252.14 747.03 2025.03 2276.70 300.35 743.55 2025.75 2216.01 290.63 690.38 1955.59 2224.18 339.85 789.43 2086.65 2167.34 Center Pixel Coordinates: 2000.00 80.42755179994 1642.00 -68.85227719754
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-p2050a-f-3057x3281.tif
Metadata Date
2020-10-13T09:20:21-04:00
Metadata Version
1.2
×

 

Detailed color mapping information coming soon...

×
Universescalefull
168,000 light years

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