Share

News Release Archive:

News Release 229 of 959

September 9, 2009 11:00 AM (EDT)

News Release Number: STScI-2009-25

Hubble Opens New Eyes on the Universe

Back

Image: Fingerprinting the Distant Universe Using the Light from Quasar PKS 0405-123

Fingerprinting the Distant Universe Using the Light from Quasar PKS 0405-123STScI-PRC2009-25g

Screen-use options: These files are created for viewing on your monitor

Print-use download options: These files are designed to fit on letter-size paper


ABOUT THIS IMAGE:

Using a distant quasar as a cosmic flashlight, a new instrument aboard NASA's Hubble Space Telescope has begun probing the invisible, skeletal structure of the universe.

Called the cosmic web, it is the diffuse, faint gas located in the space between galaxies. More than half of all normal matter resides outside of galaxies. By observing the cosmic web, astronomers can probe the raw materials from which galaxies form, and determine how this gas was assembled into the complex structures of the present-day universe.

Using the light from the quasar PKS 0405-123, located 7 billion to 8 billion light-years away, the newly installed Cosmic Origins Spectrograph (COS) on Hubble probed a string of gas clouds residing along the light path at different distances. Quasars are the bright cores of active galaxies and are powered by supermassive black holes. Thousands of quasars have been observed, all at extreme distances from our Milky Way galaxy. The most luminous quasars radiate at a rate equivalent to a trillion suns.

The COS spectrum shown here reveals the absorption lines of elements that make up the intervening gas clouds traversed by the quasar's light. COS detected three to five times more lower-density filaments of hydrogen in the cosmic web than were seen in previous observations along this line of sight. The instrument also detected evidence of glowing oxygen and nitrogen that predominantly trace strong shocks in the filamentary cosmic web.

These shocks are produced by gravitational interactions between intergalactic clouds of gas falling onto filaments in the web and by the fast outflow of material from star-forming galaxies.

COS produced this spectrum and detected many previously unseen filaments in only a quarter of the time it took to produce spectra in previous studies of this object (using earlier instruments). The spectrum is also of higher quality (with a better signal-to-noise ratio) than those spectra produced by the best previous observations.

With the COS, astronomers have access to thousands of quasars where only a handful could be observed before in the ultraviolet. Each quasar sightline passes through multiple filaments of the cosmic web, providing a picture of how intergalactic spaces evolve over time, as light passes from the quasar to us.

These data are the first in a series of large observation programs that will map out the cosmic web. The studies will trace the complex cycles of how material flows between galaxies and intergalactic space.

COS observed the quasar in far-ultraviolet light in August 2009. The instrument was installed by NASA astronauts in May 2009, during the servicing mission to upgrade and repair the 19-year-old Hubble telescope.

These Hubble observations of the quasar PKS 0405-123 are part of the Hubble Servicing Mission 4 Early Release Observations.

Object Name: PKS 0405-123

Image Type: Astronomical/Illustration

Credit: NASA, ESA, the Hubble SM4 ERO Team, and Digitized Sky Survey

Technical facts about this image:

About this Object
Object Name: PKS 0405-123
Object Description: Quasar/Active Galaxy
Position (J2000): R.A. 04h 07m 48s.43
Dec. -12° 11' 36".66
Constellation: Eridanus
Distance: 7billion-8 billion light-years (~2 billion parsecs)
About these Data
Data Description: The Hubble spectrum was created from data from proposal 11508: K. Noll (STScI) and J. Green, C. Froning, and B. Keeney (University of Colorado, Boulder). The DSS image is courtesy of the Digitized Sky Survey, STScI/AURA, Palomar/Caltech, and the UKSTU/AAO.
Mission/Project: Hubble Digitized Sky Survey
Instrument: COS/FUV Anglo-Australian Observatory: UK Schmidt
Exposure Date(s): August 3, 2009 November 6, 1983 and January 10, 1986
Exposure Time: 2.7 hours 2.2 hours
Filters/Gratings: G130M (130nm) Red: OG590, Blue: GG395
About this Image
Credit: NASA, ESA, the Hubble SM4 ERO Team, and DSS
Release Date: September 9, 2009
Orientation/Scale: Digitized Sky Survey Image of PKS 0405-123
Acknowledgments for PKS 0405-123
Observers: K. Noll (STScI) and J. Green, C. Froning, and B. Keeney (University of Colorado, Boulder)
Data Analysis: C. Froning and J. Green (University of Colorado, Boulder)
Image Composition: Z. Levay and L. Frattare (STScI)
Text: L. Frattare, D. Weaver, and R. Villard (STScI)
Illustrations: A. Feild and Z. Levay (STScI)
Science Consultants: M. Livio (STScI) and C. Froning and J. Green (University of Colorado, Boulder)

NEWS RELEASE IMAGES

The above montage includes these images:

Digitized Sky Survey Image of PKS 0405-123 Image Type: Astronomical Digitized Sky Survey Image of PKS 0405-123 PKS 0405-123 COS Spectrum Image Type: Illustration PKS 0405-123 COS Spectrum

All images from this news release:

To access available information and downloadable versions of images in this news release, click on any of the images below: