Hubble's Wide View of 'Mystic Mountain' in Infrared

 Hubble's Wide View of 'Mystic Mountain' in Infrared

This is a NASA Hubble Space Telescope near-infrared-light image of a three-light-year-tall pillar of gas and dust that is being eaten away by the brilliant light from nearby stars in the tempestuous stellar nursery called the Carina Nebula, located 7,500 light-years away in the southern constellation Carina. The image marks the 20th anniversary of Hubble's launch and deployment into an orbit around Earth.

The image reveals a plethora of stars behind the gaseous veil of the nebula's wall of hydrogen, laced with dust. The foreground pillar becomes semi-transparent because infrared light from background stars penetrates through much of the dust. A few stars inside the pillar also become visible. The false colors are assigned to three different infrared wavelength ranges.

Hubble's Wide Field Camera 3 observed the pillar in February and March 2010.

Credits

Image

NASA, ESA, Mario Livio (STScI), Hubble 20th Anniversary Team (STScI)

About The Object
Object Name HH 901 and HH 902 in the Carina Nebula
Object Description Carina Nebula Star-forming Pillars and Herbig-Haro Objects with Jets
R.A. Position 10h 44m 5.25s
Dec. Position -59° 29' 44.99"
Constellation Carina
Distance 7,500 light-years (2,300 parsecs)
About The Data
Data Description This image was created from HST data from proposal : M. Livio, K. Noll, M. Mutchler, Z. Levay, L. Frattare, W. Januszewski, C. Christian, and T. Borders (Hubble 20th Anniversary Team, STScI).
Instrument HST>WFC3/IR
Exposure Dates February/March 2010, Exposure Time: 12 hours
Filters F126N ([Fe II]), F128N (Paschen-beta), and F164N ([Fe II])
About The Image
Color Info This image is a composite of separate exposures made by the WFC3 instrument on the Hubble Space Telescope (HST). Each filter was used to sample a narrow wavelength range over a broad range of the visible colors. The composite color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Red: F126N ([Fe II]) Green: F128N (Paschen-beta) Blue: F164N ([Fe II])
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.