Archivo de imágenes de Hubble

Un mar de galaxias espirales

This is a Hubble Space Telescope view of a small, random location on the sky, awash largely with spiral galaxies like our Milky Way. This sea of galaxies stretches across billions of light-years. Most of the prominent galaxies look different only because they are tilted at variou...

Fecha
Jan 1, 2017
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2017-14-4021-image
Por

This is a Hubble Space Telescope view of a small, random location on the sky, awash largely with spiral galaxies like our Milky Way. This sea of galaxies stretches across billions of light-years. Most of the prominent galaxies look different only because they are tilted at various orientations to Earth, from edge-on to face-on. A few others are involved in mergers. The objects with diffraction spikes are foreground stars in our own galaxy. The image was taken with the Advanced Camera for Surveys (ACS) at the same time a much closer pair of spiral galaxies, NGC 4302 and NGC 4298, was being simultaneously photographed by Hubble's Wide Field Camera 3 (WFC3). These so-called "parallel field" observations increase the efficiency of how the telescope is used when making observations.

Credits

NASA, ESA, and M. Mutchler (STScI)

Detalles de la imagen

About The Object
Object NameParallel Field
Object DescriptionField of galaxies
R.A. Position12h21m49.4s
Dec. Position14º28'41"
ConstellationComa Berenices
DimensionsThe image is about 5 arcminutes wide.
About The Data
Data DescriptionThese datasets are from the HST proposal , M. Mutchler, J. Green, Z. Levay, D. Smith, and R. Villard (STScI), and image processing by J. DePasquale (STScI).
InstrumentHST>ACS/WFC
Exposure DatesJan. 2 - 22, 2017
FiltersF606W
About The Image
Color InfoThis image is a composite of separate exposures made by the ACS instrument on the Hubble Space Telescope using the F606W (V) filter to isolating the light in broad wavelength range to produce a monochromatic image.

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Fuente

La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.

Ver en NASA.gov

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