Grayscale Image of the Tarantula Nebula

 Grayscale Image of the Tarantula Nebula

Credits

NASA, ESA, and D. Lennon (ESA/Hubble)

About The Object
Object Name Tarantula Nebula, 30 Doradus, 30 Dor, NGC 2070
Object Description Emission Nebula in the Large Magellanic Cloud
R.A. Position 05h 38m 42.36s
Dec. Position -69° 6' 3.24"
Constellation Dorado
Distance Approximately 170,000 light-years (52,000 parsecs)
Dimensions This image is roughy 14.4 arcminutes (662 light-years or 204 parsecs) wide.
About The Data
Data Description This image combines many exposures from the Hubble Space Telescope's Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3) from the HST proposal Grayscale Image of the Tarantula Nebula: D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam).
Instrument HST>ACS/WFC and HST>WFC3/UVIS
Exposure Dates October 2011
Filters ACS/WFC and WFC3/UVIS: F775W (SDSS i)
About The Image
Color Info This image is a composite of separate exposures made by the ACS and WFC3 instruments on the Hubble Space Telescope.
Compass Image Grayscale Image of the Tarantula Nebula
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The 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.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: 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.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.