Sukrit Ranjan

Assistant Professor

University of Arizona

United States

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Dr. Sukrit Ranjan is an Assistant Professor at the University of Arizona, USA. His research focuses on exoplanet atmospheres, biosignatures, and the geochemical processes that may influence habitability. Recent publications include studies on the atmospheric constraints of habitable zone planets and the impacts of various gases on temperate anoxic atmospheres.

Articles (16)

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2025

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2023

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2022

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2022

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2022

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2021

Collaborators (6)

Clara Sousa-Silva

Assistant Professor

Bard College

UNITED STATES

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Hannah Wakeford

University of Bristol

UNITED KINGDOM

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Corinna L. Kufner

Harvard University

UNITED STATES

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Kevin Stevenson

Professional Staff

Johns Hopkins University Applied Physics Laboratory

UNITED STATES

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P. B. Rimmer

University of Cambridge

UNITED KINGDOM

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Lisa Kaltenegger

Director Carl Sagan Institute Cornell, Professor

Cornell University

UNITED STATES

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Sukrit Ranjan

Research Interests

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About

Articles (16)

JWST-TST DREAMS: Secondary Atmosphere Constraints for the Habitable Zone Planet TRAPPIST-1 e

Bioverse: Potentially Observable Exoplanet Biosignature Patterns under the UV Threshold Hypothesis for the Origin of Life

The Impact of Extended CO2 Cross Sections on Temperate Anoxic Planet Atmospheres

The Impact of Extended H2O Cross Sections on Temperate Anoxic Planet Atmospheres: Implications for Spectral Characterization of Habitable Worlds

UV Spectral Characterization of Low-mass Stars with AstroSat UVIT for Exoplanet Applications: The Case Study of HIP 23309

Geochemical and Photochemical Constraints on S[IV] Concentrations in Natural Waters on Prebiotic Earth

The Importance of the Upper Atmosphere to CO/O2 Runaway on Habitable Planets Orbiting Low-mass Stars

Venusian phosphine: a ‘wow!’ signal in chemistry?

H2-dominated Atmosphere as an Indicator of Second-generation Rocky White Dwarf Exoplanets

Methanol—A Poor Biosignature Gas in Exoplanet Atmospheres

Can Carbon Fractionation Provide Evidence for Aerial Biospheres in the Atmospheres of Temperate Sub-Neptunes?

Organic Carbonyls Are Poor Biosignature Gases in Exoplanet Atmospheres but May Generate Significant CO

Photochemical Runaway in Exoplanet Atmospheres: Implications for Biosignatures

Assessment of Ammonia as a Biosignature Gas in Exoplanet Atmospheres

Constraints on the Production of Phosphine by Venusian Volcanoes

UV Transmission in Natural Waters on Prebiotic Earth

Collaborators (6)

Clara Sousa-Silva

Hannah Wakeford

Corinna L. Kufner

Kevin Stevenson

P. B. Rimmer

Lisa Kaltenegger

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