Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Videos

Planetary atmosphere evolution: do other habitable planets exist and can we detect them?

J F Kasting1

  • 1Department of Geosciences, Penn State University, University Park, PA 16802, USA.

Astrophysics and Space Science
|January 1, 1996
PubMed
Summary

Detecting Earth-like planets, potentially habitable or inhabited, around other stars is a key goal. This research explores the likelihood of habitable exoplanets and optimal detection methods within decades.

Related Concept Videos

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Comparison between ozone column depths and methane lifetimes computed by one- and three-dimensional models at different atmospheric O<sub>2</sub> levels.

Royal Society open science·2023
Same author

Greenhouse warming by nitrous oxide and methane in the Proterozoic Eon.

Geobiology·2011
Same author

Low pCO2 in the pore water, not in the Archean air.

Nature·2011
Same author

Mass-independent fractionation of sulfur isotopes in Archean sediments: strong evidence for an anoxic Archean atmosphere.

Astrobiology·2002
Same author

Irradiated interplanetary dust particles as a possible solution for the deuterium/hydrogen paradox of Earth's oceans.

Journal of geophysical research·2001
Same author

Synthetic spectra of simulated terrestrial atmospheres containing possible biomarker gases.

Icarus·2001

Area of Science:

  • Exoplanetary science
  • Astrobiology
  • Planetary atmosphere evolution

Background:

  • The search for extraterrestrial life hinges on detecting Earth-like planets.
  • Defining "Earth-like" includes habitability and potential for life.

Purpose of the Study:

  • To assess the probability of habitable exoplanets existing around other stars.
  • To determine the most effective methods for detecting inhabited exoplanets.

Main Methods:

  • Utilizing ground-based and space-based telescopes and interferometers.
  • Analyzing planetary atmosphere evolution models.

Main Results:

  • The study considers the feasibility of detecting Earth-like exoplanets in the coming decades.
Keywords:
NASA Discipline ExobiologyNon-NASA Center

Related Experiment Videos

  • It addresses the probability of habitable and inhabited exoplanets.
  • Conclusions:

    • The conference aims to evaluate the possibility of detecting Earth-like exoplanets.
    • Key questions involve the prevalence of habitable worlds and detection strategies.