output
20112026
most citedHabitable Zones Around Main-Sequence Stars: Dependence on Planetary Mass

675 citations

Showing 2017Show all

13 papers · 1 filter

astro-ph.EP2017★ 11 cited

EXONEST: The Bayesian Exoplanetary Explorer

Kevin H. Knuth, Ben Placek, Daniel Angerhausen +4

The fields of astronomy and astrophysics are currently engaged in an unprecedented era of discovery as recent missions have revealed thousands of exoplanets orbiting other stars. W…

astro-ph.SR2017★ 5 cited

The year-long flux variations in Boyajian's star are asymmetric or aperiodic

Michael Hippke, Daniel Angerhausen

We combine and calibrate publicly available data for Boyajian's star including photometry from ASAS (SN, V, I), Kepler, Gaia, SuperWASP, and citizen scientist observations (AAVSO,…

astro-ph.EP2017★ 125 cited

Demarcating circulation regimes of synchronously rotating terrestrial planets within the habitable zone

Jacob Haqq-Misra, Eric. T. Wolf, Manoj Joshi +2

We investigate the atmospheric dynamics of terrestrial planets in synchronous rotation within the habitable zone of low-mass stars using the Community Atmosphere Model (CAM). The s…

astro-ph.EP2017★ 4 cited

Simultaneous multicolour optical and near-IR transit photometry of GJ 1214b with SOFIA

D. Angerhausen, C. Dreyer, B. Placek +24

The benchmark exoplanet GJ 1214b is one of the best studied transiting planets in the transition zone between rocky Earth-sized planets and gas or ice giants. This class of super-E…

physics.pop-ph2017★ 7 cited

The Drake Equation as a Function of Spectral Type and Time

Jacob Haqq-Misra, Ravi Kumar Kopparapu

This chapter draws upon astronomical observations and modeling to constrain the prevalence of communicative civilizations in the galaxy. We discuss the dependence of the Drake equa…

physics.pop-ph2017★ 30 cited

Why do we find ourselves around a yellow star instead of a red star?

Jacob Haqq-Misra, Ravi Kumar Kopparpu, Eric T. Wolf

M-dwarf stars are more abundant than G-dwarf stars, so our position as observers on a planet orbiting a G-dwarf raises questions about the suitability of other stellar types for su…

astro-ph.EP2017★ 326 cited

Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment

Victoria S. Meadows, Christopher T. Reinhard, Giada N. Arney +13

Here we review how environmental context can be used to interpret whether O2 is a biosignature in extrasolar planetary observations. This paper builds on the overview of current bi…

astro-ph.EP2017★ 205 cited

Habitable Moist Atmospheres On Terrestrial Planets Near the Inner Edge Of the Habitable Zone Around M-dwarfs

Ravi kumar Kopparapu, Eric T. Wolf, Giada Arney +4

Terrestrial planets in the habitable zones (HZs) of low-mass stars and cool dwarfs have received significant scrutiny recently because their shorter orbital periods increase their…

astro-ph.EP2017★ 131 cited

Exoplanet Biosignatures: Future Directions

Sara I. Walker, William Bains, Leroy Cronin +11

Exoplanet science promises a continued rapid accumulation of new observations in the near future, energizing a drive to understand and interpret the forthcoming wealth of data to i…

astro-ph.EP2017★ 168 cited

Exoplanet Biosignatures: Observational Prospects

Yuka Fujii, Daniel Angerhausen, Russell Deitrick +9

Exoplanet hunting efforts have revealed the prevalence of exotic worlds with diverse properties, including Earth-sized bodies, which has fueled our endeavor to search for life beyo…

astro-ph.EP2017★ 529 cited

Exoplanet Biosignatures: A Review of Remotely Detectable Signs of Life

Edward W. Schwieterman, Nancy Y. Kiang, Mary N. Parenteau +15

In the coming years and decades, advanced space- and ground-based observatories will allow an unprecedented opportunity to probe the atmospheres and surfaces of potentially habitab…

astro-ph.EP2017★ 95 cited

Constraints on Climate and Habitability for Earth-like Exoplanets Determined from a General Circulation Model

Eric T. Wolf, Aomawa L. Shields, Ravi K. Kopparapu +2

Conventional definitions of habitability require abundant liquid surface water to exist continuously over geologic timescales. Water in each of its thermodynamic phases interacts w…

astro-ph.EP2017★ 93 cited

False negatives for remote life detection on ocean-bearing planets: Lessons from the early Earth

C. T. Reinhard, S. L. Olson, E. W. Schwieterman +1

Ocean-atmosphere chemistry on Earth has undergone dramatic evolutionary changes through its long history, with potentially significant ramifications for the emergence and long-term…