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Hubble Observes Blue Stars in Andromeda’s Core

The image at left shows the nearby, majestic Andromeda galaxy. The rectangular box marks the region probed by NASA's Hubble Space Telescope.
Hubble's view, taken with the Wide Field Camera 3 and the Advanced Camera for Surveys, is shown in the images on the right. The images are a blend of visible and ultraviolet light. The photo at top right is 7,900 light-years across and reveals the galaxy's crowded central region. The bright area near the center of the image is a grouping of stars nestled around the galaxy's black hole. The blue dots sprinkled throughout the image are ultra-blue stars whose population increases around the crowded hub. The blue stars are old Sun-like stars that have prematurely cast off their outer layers of material, exposing their extremely blue-hot cores. The square box outlines a close-up view of an area around the core.
The detailed image, shown at bottom right, reveals a richer population of blue stars huddled around the core. Dark dust clouds also are visible. The image is 740 light-years wide.
The right-hand images, taken with Hubble, are part of a census of stars in M31 called the Panchromatic Hubble Andromeda Treasury survey.
The image of the Andromeda galaxy was taken on June 13, 2001, with the WIYN/KPNO 0.9-meter Mosaic I by T. Rector and B. Wolpa of the National Optical Astronomy Observatory in Tucson, Ariz.
Hubble images: NASA, ESA, B.F. Williams (University of Washington, Seattle), D. Lang (Princeton University, N.J.), J. Kalirai (Space Telescope Science Institute, Baltimore), and J. Dalcanton (University of Washington, Seattle)
WIYN/KPNO Image: T. Rector and B. Wolpa (NOAO/AURA/NSF)
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.00h 42m 44.0s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.41° 16' 8.99"
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Andromeda
- DistanceDistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.About 2.5 million light-years (0.8 megaparsecs)
About the Data
- Data DescriptionData DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.The Panchromatic Hubble Andromeda Treasury (PHAT) survey of M31 is an ongoing HST Treasury proposal. These inset images were created from Hubble data from proposal 12058 (PI: J. Dalcanton, University of Washington, Seattle).
- InstrumentInstrumentThe science instrument used to produce the data.WIYN/KPNO>0.9m (galaxy image), and HST>WFC3/UVIS, HST>WFC3/IR, and HST>ACS/WFC (inset images)
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.Data used in these images were taken in 2010 and 2011.
- FiltersFiltersThe camera filters that were used in the science observations.Hubble Image (inset images): WFC3/UVIS: F275W (UV) and F336W (U)ACS/WFC: F475W (g) and F814W (I)WFC3/IR: F160W (H)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.M31, NGC 224, Andromeda Galaxy, and PHAT Treasury Survey Region of M31 (inset images)
- Object DescriptionObject DescriptionThe type of astronomical object.PHAT Treasury Survey Region of M31
- Release DateJanuary 11, 2012
- Science ReleaseRare Ultra-blue Stars Found in Neighboring Galaxy’s Hub
- CreditsNASA, ESA, Benjamin Williams (UWashington), D. Lang (Princeton University), Jason Kalirai (STScI), Julianne Dalcanton (UWashington), Travis Rector (NOAO, AURA, NSF), B. Wolpa (NOAO, AURA, NSF)

Wide M31 Image (top inset image)Blue: F336W(U)Cyan: F475W (g)Yellow: F814W(I)Red: F160W (H) (H) Detail M31 Image (bottom inset image)Light purple: F275W (UV)Blue: F336W (U)ACS/WFC: F475W (g)Dark red: F814W (I)
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov