Carl Sagan Institute

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The Carl Sagan Institute: Pale Blue Dot and Beyond was founded in 2014 at Cornell University in Ithaca, New York to further the search for habitable planets and moons in and outside the Solar System. It is focused on the characterization of exoplanets and the instruments to search for signs of life in the universe.[1][2] The founder and current director of the institute is astronomer Lisa Kaltenegger.

The Institute, inaugurated in 2014 and renamed on 9 May 2015, collaborates with international institutions on fields as astrophysics, engineering, earth and atmospheric science, geology and biology with the goal of taking an interdisciplinary approach to the search for life elsewhere in the universe and of the origin of life on Earth.[1][3]

Carl Sagan was a faculty member at Cornell University beginning in 1968. He was the David Duncan Professor of Astronomy and Space Sciences and director of the Laboratory for Planetary Studies there until his death in 1996.[1]

Research[edit | hide | hide all]

The main goal of the Carl Sagan Institute is to model atmospheric spectral signatures including biosignatures, of known and hypothetical planets and moons to explore whether they could be habitable and how they could be detected.[4] Their research focuses on exoplanets and moons orbiting in the habitable zone around their host stars. The atmospheric characterization of such worlds would allow to potentially detect the first habitable exoplanet.[4] A team member has already produced a "color catalog" that could help scientists look for signs of life on exoplanets.[5]

Bioreflectance spectra catalog[edit | hide]

Team scientists used 137 different microorganism species, including extremophiles that were isolated from Earth's most extreme environments, and cataloged how each life form uniquely reflects sunlight in the visible and near-infrared to the short-wavelength infrared (0.35–2.5 µm) portions of the electromagnetic spectrum.[6] This database of individual reflection 'fingerprints' (spectrum) might be used by astronomers as biosignatures to find large colonies of microscopic life on distant exoplanets.[5] A combination of organisms would produce a mixed spectrum, also cataloged, of light bouncing off the planet. The goal of the catalog is to provide astronomers with a baseline comparison to help scientists interpret the data that will come back from telescopes like WFIRST and E-ELT.[5]

See also[edit | hide]

References[edit | hide]

  1. 1.0 1.1 1.2 Cofield, Calla (9 May 2015). "Institute for Pale Blue Dots Renamed to Honor Carl Sagan, Will Search for Alien Life". Retrieved 2015-05-11. 
  2. "About the Carl Sagan Institute". 8 May 2015. Retrieved 2015-05-11. 
  3. Glaser, Linda (January 27, 2015). "Introducing: The Carl Sagan Institute". Archived from the original on 2015-02-27. Retrieved 2015-05-11. 
  4. 4.0 4.1 "Carl Sagan Institute - Research". May 2015. Retrieved 2015-05-11. 
  5. 5.0 5.1 5.2 Cofield, Calla (30 March 2015). "Catalog of Earth Microbes Could Help Find Alien Life". Retrieved 2015-05-11. 
  6. Hegde, Siddharth; Paulino-Lima, Ivan G.; Kent, Ryan; Kaltenegger, Lisa; Rothschild, Lynn (31 March 2015). "Surface biosignatures of exo-Earths: Remote detection of extraterrestrial life". PNAS. 112 (13): 3886–3891. Bibcode:2015PNAS..112.3886H. doi:10.1073/pnas.1421237112. PMC 4386386Freely accessible. PMID 25775594. Retrieved 2015-05-11. 

Coordinates: 42°26′55″N 76°28′43″W / 42.448510°N 76.478620°W / 42.448510; -76.478620

This article uses material from Carl Sagan Institute on Wikipedia (view authors). License under CC BY-SA 3.0. Wikipedia logo
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