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Executive Summary: The Habitable Worlds Observatory (HWO) is the first astrophysics flagship mission with a key cross-divisional astrobiology science goal of searching for signs of life on rocky planets beyond our solar system. The Living…

Modeling the detection of life has never been more opportune. With next generation space telescopes, like the currently developing Habitable Worlds Observatory (HWO) concept, we will begin to characterize rocky exoplanets potentially…

Earth and Planetary Astrophysics · Physics 2024-04-26 Schuyler R. Borges , Gabrielle G. Jones , Tyler D. Robinson

Searching for signs of life is a primary goal of the Habitable Worlds Observatory (HWO). However, merely detecting oxygen, methane, or other widely discussed biosignatures is insufficient evidence for a biosphere. In parallel with…

The Habitable Worlds Observatory (HWO) aims to characterize habitable exoplanets in search of signs of life. However, detectable life may be rare, either because abiogenesis is intrinsically contingent and unlikely, or because biospheres…

Instrumentation and Methods for Astrophysics · Physics 2025-07-02 Sukrit Ranjan , Danica Adams , Michael Wong , Martin Schlecker , Nicholas Wogan , Jessica M. Weber

Characterizing the surface and atmosphere of Earth-like planets in reflected light is a key goal for upcoming direct imaging surveys. NASA's next flagship-class astrophysics mission concept, the Habitable Worlds Observatory (HWO), is a…

Earth and Planetary Astrophysics · Physics 2026-03-27 Aiden S. Zelakiewicz , Elijah Mullens , Lisa Kaltenegger , Dmitry Savransky

Exoplanet atmosphere characterization has seen revolutionary advances over the last few years, providing us with unique insights into atmospheric chemistry, dynamics and planet formation mechanisms. However, true solar system analog planets…

Instrumentation and Methods for Astrophysics · Physics 2026-01-13 Joanna K. Barstow , Beth Biller , Mei Ting Mak , Sarah Rugheimer , Amaury Triaud , Hannah R. Wakeford

The detection of life on rocky exoplanets in the habitable zones of nearby stars would be a paradigm-shifting advance, and it is one of the greatest scientific challenges of our time. There is no single spectral feature that is an…

Our Earth, being the only living planet that we know, provides us with clues that photosynthetic life-forms may be dominant on other exoplanets for billions of years. Spectropolarimetric signatures of the terrestrial photosynthetic life…

The Habitable Worlds Observatory (HWO) aims to telescopically constrain the frequency and abundance of biospheres in the solar neighborhood. Origin-of-life theories vary in their predictions for the environmental requirements and the…

Instrumentation and Methods for Astrophysics · Physics 2025-07-02 Sukrit Ranjan , Martin Schlecker , Nicholas Wogan , Michael Wong

The search for technosignatures--remotely detectable evidence of extraterrestrial technology--draws upon examples from the recent history of Earth as well as projections of Earth's technosphere. Facilities like the Habitable Worlds…

Earth and Planetary Astrophysics · Physics 2025-12-09 Jacob Haqq-Misra , Ravi Kopparapu , George Profitiliotis

Future direct-imaging flagship missions, such as NASA's Habitable Worlds Observatory (HWO), face critical decisions in prioritizing observations due to extremely stringent time and resource constraints. In this paper, we introduce two…

Machine Learning · Computer Science 2026-01-21 Mark Moussa , Amber V. Young , Brianna Isola , Vasuda Trehan , Michael D. Himes , Nicholas Wogan , Giada Arney

A primary goal of the Habitable Worlds Observatory (HWO) is to detect and measure the abundance of biosignature molecules, such as water (H2O) and oxygen (O2), in the atmosphere of Earth analogs. This is expected to require deep…

Habitable Worlds Observatory (HWO) will search for biosignatures from Earth-size exoplanets in the habitable zones of nearby stars. The wavelength range for biosignatures used by the HabEx and LUVOIR mission concept studies was 200 nm to 2…

The search for life outside our solar system is at the forefront of modern astronomy, and telescopes such as the Habitable Worlds Observatory (HWO) are being designed to identify biosignatures. Molecular oxygen, O$_2$, is considered a…

Earth and Planetary Astrophysics · Physics 2025-09-12 Anna Grace Ulses , Joshua Krissansen-Totton , Tyler D. Robinson , Victoria Meadows , David C. Catling , Jonathan J. Fortney

The Habitable Worlds Observatory (HWO), planned for launch in the 2040s, represents the next major step in exoplanet characterisation. HWO will, for the first time, enable detailed studies of the atmospheres and surfaces of Earth-like…

Instrumentation and Methods for Astrophysics · Physics 2026-01-30 Katy L. Chubb , Mei Ting Mak , Joanna K. Barstow , Beth Biller , Sarah Rugheimer , Daphne M. Stam , Victor Trees

NASA's Habitable Worlds Observatory (HWO) aims to achieve starlight suppression to the $10^{-10}$ level for the detection and spectral characterization of Earth-like exoplanets. Broadband ozone absorption features are key biosignatures that…

Constraints on the masses of exoplanets directly imaged and characterized by the Habitable Worlds Observatory (HWO) are crucial for categorizing these planets and interpreting their spectra. In particular, achieving a mass measurement with…

Instrumentation and Methods for Astrophysics · Physics 2026-03-13 Kaz Gary , B. Scott Gaudi , Eduardo Bendek , Tyler Robinson , Renyu Hu , Breann Sitarski , Aki Roberge , Eric Mamajek

The proposed Habitable Worlds Observatory is intended to observe the atmospheres of nearby terrestrial exoplanets with a resolution greater than that of any previous instrument. While these observations present a substantial opportunity for…

Instrumentation and Methods for Astrophysics · Physics 2025-01-14 Theresa Fisher , Chester Harman , Estelle Janin , Megan Shabram , Shang-Min Tsai , Nicholas Wogan , Michael Wong

As part of NASA's mission to explore habitable planets orbiting nearby stars, this paper explores the detection and characterization capabilities of a 4-m space telescope plus 50-m starshade located at the Earth-Sun L2 point, a.k.a. the New…

Instrumentation and Methods for Astrophysics · Physics 2015-06-04 Margaret C. Turnbull , Tiffany Glassman , Aki Roberge , Webster Cash , Charley Noecker , Amy Lo , Brian Mason , Phil Oakley , John Bally
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