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Related papers: The Color of Habitability

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A habitable exoplanet is a world that can maintain stable liquid water on its surface. Techniques and approaches to characterizing such worlds are essential, as performing a census of Earth-like planets that may or may not have life will…

Earth and Planetary Astrophysics · Physics 2024-01-22 Tyler D. Robinson

The discovery of planets orbiting stars other than the Sun has accelerated over the past decade, and this trend will continue as new space- and ground-based observatories employ next-generation instrumentation to search the skies for…

Earth and Planetary Astrophysics · Physics 2019-09-11 Aomawa L. Shields

Habitability is a measure of an environment's potential to support life, and a habitable exoplanet supports liquid water on its surface. However, a planet's success in maintaining liquid water on its surface is the end result of a complex…

Earth and Planetary Astrophysics · Physics 2021-12-15 Ravi kumar Kopparapu , Eric T. Wolf , Victoria S. Meadows

The search for extrasolar planets has already detected rocky planets and several planetary candidates with minimum masses that are consistent with rocky planets in the habitable zone of their host stars. A low-resolution spectrum in the…

Earth and Planetary Astrophysics · Physics 2015-07-30 Siddharth Hegde , Lisa Kaltenegger

Dozens of habitable zone, approximately earth-sized exoplanets are known today. An emerging frontier of exoplanet studies is identifying which of these habitable zone, small planets are actually habitable (have all necessary conditions for…

The aim of my dissertation is to investigate habitability in extra-Solar Systems. Most of the time, only planets are considered as possible places where extraterrestrial life can emerge and evolve, however, their moons could be inhabited,…

Earth and Planetary Astrophysics · Physics 2017-04-26 Vera Dobos

Earth is the only planet known to harbor life and, as a result, the search for habitable and inhabited planets beyond the Solar System commonly focuses on analogs to our planet. However, Earth's atmosphere and surface environment have…

Earth and Planetary Astrophysics · Physics 2019-10-17 Tyler D. Robinson , Christopher T. Reinhard

The detection of exoplanets orbiting other stars has revolutionized our view of the cosmos. First results suggest that it is teeming with a fascinating diversity of rocky planets, including those in the habitable zone. Even our closest…

Earth and Planetary Astrophysics · Physics 2019-11-20 L. Kaltenegger

The search for life beyond the Solar System remains a primary goal of current and near-future missions, including NASA's upcoming Habitable Worlds Observatory (HWO). However, research into determining the habitability of terrestrial…

Large ground- and space-based telescopes will be able to observe Earth-like planets in the near future. We explore how different planetary surfaces can strongly influence the climate, atmospheric composition, and remotely detectable spectra…

Earth and Planetary Astrophysics · Physics 2020-05-20 Jack Madden , Lisa Kaltenegger

The dynamic nature of life's ability to thrive in diverse and changing planetary environments suggests that habitability and survival depend on the evolutionary path and life adaptation to environmental conditions. Here we explore such…

Earth and Planetary Astrophysics · Physics 2024-07-04 Itay Weintraub , Hagai B. Perets

As of 2025, over 6000 planets are known to orbit stars other than our Sun. We can measure their sizes and orbital periods, infer their masses and temperatures, and constrain their compositions. Based on these data, about 1% of extrasolar…

Astrophysics of Galaxies · Physics 2025-10-13 Floris van der Tak

In the past 15 years, astronomers have revealed that a significant fraction of the stars should harbor planets and that it is likely that terrestrial planets are abundant in our galaxy. Among these planets, how many are habitable, i.e.…

Earth and Planetary Astrophysics · Physics 2013-05-09 Francois Forget

Planets with large bodies of water on their surface will have more temperate and stable climates, and such planets are the ideal places for life-as-we-know-it to arise and evolve. A key science case for the Habitable Worlds Observatory…

Instrumentation and Methods for Astrophysics · Physics 2025-07-08 Nicolas B. Cowan , Jacob Lustig-Yaeger , Renyu Hu , Laura C. Mayorga , Tyler D. Robinson

This article reviews the emerging field of exo-geoscience, focusing on the geological and geophysical processes thought to influence the evolution and (eu)habitability of rocky exoplanets. We examine the possible roles of planetary…

Earth and Planetary Astrophysics · Physics 2026-01-21 Tilman Spohn , Akli Roberge , M. J. Way , João C. Duarte , Francesca Miozzi , Philipp Baumeister , Paul Byrne , Charles Lineweaver

In this paper we discuss how we can read a planets spectrum to assess its habitability and search for the signatures of a biosphere. After a decade rich in giant exoplanet detections, observation techniques have now reached the ability to…

Earth and Planetary Astrophysics · Physics 2015-05-13 L. Kaltenegger , F. Selsis , M. Fridlund , H. Lammer , the Darwin Science team

The investigation of exoplanetary habitability is integral to advancing our knowledge of extraterrestrial life potential and detailing the environmental conditions of distant worlds. In this analysis, we explore the properties of exoplanets…

Earth and Planetary Astrophysics · Physics 2024-08-20 Jonathan H. Jiang , Philip E. Rosen , Christina X. Liu , Qianzhuang Wen , Yanbei Chen

The characteristics of irradiated solar system planetary atmospheres have been studied for decades, consequently modern planetary science benefits from an exhaustive body of ground- and space-based data. The study of extrasolar planetary…

Astrophysics · Physics 2008-09-29 Mark S. Marley

The detection of massive planets orbiting nearby stars has become almost routine, but current techniques are as yet unable to detect terrestrial planets with masses comparable to the Earth's. Future space-based observatories to detect…

Astrophysics · Physics 2015-06-24 E. B. Ford , S. Seager , E. L. Turner
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