Posts Tagged 'Advent 2012'

My Gift to You (Science Christmas)

(Here ends Science Advent, in which I posted a science-related image every day.)

Christmas Day

The multicolored Universe. Click for the larger version. [Credit: moi (mosaic); see below for others]

The gift we all possess: our multicolored Universe. Click for the larger version. [Credit: moi (mosaic); see below for others]

Today my gift to you is something we all possess: our Universe. The image above shows the whole sky in many different kinds of light. Visible light is what we can see with our eyes; the view is dominated by the disk of the Milky Way, our galactic home. However, visible light is only a narrow portion of the total spectrum. The two pictures immediately below are different wavelengths of infrared (IR) light that emphasize many different sources, including emission from dust. The gamma ray and X-ray images pick out neutron stars, black holes, supernova remnants, and other bright energetic phenomena. Hydrogen is the most common element in the Universe, and it emits light in the radio portion of the spectrum.

However, as a cosmologist, I most love the final image: the sky in microwave light. While the visible, infrared, radio, gamma-ray, and X-ray emissions show us a Universe as it is today—stars, dust, gas, and galaxies—the microwave sky reveals our origins. The colors in that image represent tiny fluctuations from when the Universe was less than 400,000 years old. Those fluctuations over time grew to become galaxies. Our beginnings are marked out in these colors. The Universe’s past and present are revealed in these images.

Image credits:

  • Visible light is a mosaic from many Earth-based perspectives. Credit: Axel Mellinger
  • 9 micron (infrared) light, seen by the Japanese AKARI satellite. Credit: JAXA/AKARI
  • dust and stellar IR colors: the blue-green is light represents stars and galaxies at 3.4 microns. The green color is 12 microns, while the red is 22 microns, both emitted by dust. All of these were imaged by the WISE satellite. Credit: NASA/JPL-Caltech/UCLA
  • gamma-ray light was from a survey by the Fermi orbiting observatory. Credit: NASA/DOE/Fermi LAT Collaboration
  • the colors in the X-ray image come from three different instruments on the ROSAT satellite. Credit: Max-Planck-Institut für extraterrestrische Physik
  • hydrogen emits light at 21 centimeters of wavelength, which is in the radio portion of the spectrum. Credit: NRAO/AUI
  • finally, the microwave sky is known as the cosmic microwave background (CMB), which I wrote about in a previous entry. Credit: NASA/WMAP Science Team


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