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HST PHAT Detail of M31
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.HST>WFC3/UVIS, HST>WFC3/IR, and HST>ACS/WFC
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.2010 and 2011
- FiltersFiltersThe camera filters that were used in the science observations.WFC3/UVIS: F275W (UV) and F336W (U)ACS/WFC: F475W (g) and F814W (I)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.M31, NGC 224, Andromeda Galaxy detail
- 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), Julianne Dalcanton (UWashington)
This image is a composite of separate exposures acquired by the WFC3 and ACS instruments on HST. Several filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are:Detail M31 Image (at bottom)Light purple: F275W (UV)Blue: F336W (U)Green: F475W (g)Dark red: F814W (I)
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov