![Schematic diagram of the simulated architecture. It includes the segmented primary mirror, an APLC coronagraph with an apodizer, a focal plane mask and a Lyot stop, two deformable mirrors, and an out-of-band and a low-order Zernike wavefront sensor. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/JWST-telemetry.png?resize=1200%2C712&ssl=1)
[astro-ph.IM] We provide a quantification of the technological gap between the James Webb Space Telescope (JWST) and the Habitable Worlds Observatory (HWO) for the goal of exo-Earth imaging around Sun-like […]
Habitable Worlds Observatory
![Cumulative oxygen loss for planets at the habitable zone of each sample star over 1 Gyr, assuming constant stellar XUV flux at the HZ and no replenishment of oxygen. The curves are calculated using the energy-limited O2 loss prescription from V. S. Airapetian et al. 2017. Colored lines show individual stars, with solid segments representing the earliest ages (for stars with age ranges) and dashed segments extending beyond the minimum age. The black solid line shows the solar reference. Horizontal lines indicate the present-day Earth atmospheric O2 content (∼0.2 bars; dotted) and the total mass of Earth’s oceans (∼240 bars; dashed), providing reference levels for planetary habitability. -- [astro-ph.SR]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Panchromatic.png?resize=1200%2C720&ssl=1)
Posted inHabitable Zones
Panchromatic Spectra of Nearby Low-mass and Sun-like Stars with Directly Imageable Habitable Zones
[astro-ph.SR] Characterizing the high-energy radiation environments of stars plays a critical role in determining which systems’ planets are capable of retaining atmospheres and sustaining habitable conditions.
![Earth biosignatures through time and their reflected light spectra. The left subplot shows estimates of Earth’s bulk atmospheric composition through time (advancing from top to bottom), and the figures on the right show the corresponding reflected light spectra considered in this study. Key absorption features for biosignature gases (O3, O2, CH4) and suggested long- and short-wavelength cutoffs are highlighted (as discussed further in Sections 3 and 4). Adapted from National Academies of Sciences, Engineering, and Medicine (2021) and LUVOIR and HabEx Final Reports (LUVOIR Team, 2019; Gaudi et al., 2020). -- [Astrobiology (Journal)]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Wavelength.png?resize=1200%2C719&ssl=1)
Posted inBiosignatures & Paleobiology
Wavelength Requirements for Life Detection via Reflected Light Spectroscopy of Rocky Exoplanets
[Astrobiology (Journal)] 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 […]
Posted inBiosignatures & Paleobiology
The Effects of M Star Age Dependent Ultraviolet Emission on Detecting and Interpreting Exoplanet Biosignatures
[astro-ph.EP] Given their abundance and observational advantages, M stars will arguably be the best candidates for characterizing and searching for biosignatures on terrestrial exoplanets in the near future.
Posted inHabitable Zones
Planetary Stability and Long-Term Habitability in Nearby Stellar Binaries: 70 Oph, 36 Oph, γ Leo
[astro-ph.EP] Binary stars are common and have the potential to host habitable planets, which may reside in more complex habitable zones as compared to planets orbiting single stars.
Posted inPress Release
Habitable Worlds Observatory’s Concept and Technology Maturation: Initial Feasibility and Trade Space Exploration
[astro-ph.IM] The Habitable Worlds Observatory is the first telescope ever designed to search for life and will be a powerhouse of discovery across topics in astrophysics.
Posted inAstronomy & Telescopes
NASA ROSES-25 Amendment 69: New Opportunity: D.9 Habitable Worlds Observatory Instrument Concept Assessments
[NASA] Habitable Worlds Observatory (HWO) Instrument Concept Assessments (HWO-ICA) program element D.9 of ROSES-25, solicits proposals to support maturation of the HWO mission concept. The objective of HWO-ICA is to […]
![Mapping of the science cases proposed by the Science Working Groups (center) to the questions and discovery areas identified by Astro2020 (left and right). The transparencies of the lines indicate the number of connections with darker lines indicating stronger links between the SWG and the Astro2020 topic. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Early-Exploration.png?resize=1200%2C711&ssl=1)
Posted inAstronomy & Telescopes
Early Exploration Of The Scientific Discovery Space For The Habitable Worlds Observatory
[astro-ph.IM] The Habitable Worlds Observatory (HWO) is a future NASA flagship mission concept identified by the Astro2020 Decadal Survey as the highest priority for large space missions. HWO should conduct […]
![Representative spectral energy distribution fits for four HWO ExEP target stars: HD 2151 (upper left), HD 3651 A (upper right), HD 4813 (lower left), and HD 10700 (lower right). In each panel, the solid curve represents the best-fitting Pickles (1998) template spectrum, and the filled circles show the broadband photometry with associated uncertainties. Photometric error bars are shown in the y-direction, and filter widths in the x-direction. Fractional residuals between the template flux averaged over each bandpass and the literature photometry are shown in the lower sub-panels. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Spectral-Energy.png?resize=1200%2C716&ssl=1)
Posted inAstronomy & Telescopes
Spectral Energy Distribution Analysis For Habitable Worlds Observatory Target Stars
[astro-ph.EP] The Habitable Worlds Observatory (HWO) will directly image and characterize planets potentially similar to Earth orbiting nearby stars.
![Penalty incurred when phase is unknown, with polarimetry. The true phase set is α = (150◦, 120◦, 90◦, 60◦, 30◦, 5◦). Left: known-phase radius consequence, in which trial phases are fixed to the true set. Middle: unknown-phase radius consequence, in which trial phase tuples are marginalized over the sampled grid while the normalized I400 lightcurve shape is included with the intensive observables. Right: unknown-phase to known-phase penalty ratio. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Multiepoch.png?resize=1200%2C720&ssl=1)
Posted inAstronomy & Telescopes
Multi-epoch Ultraviolet Observables For Breaking The Radius-albedo Degeneracy In Directly Imaged Exoplanets
[astro-ph.EP] Direct imaging measures how bright a planet appears in reflected starlight, but brightness alone cannot tell whether the planet is large and dark or small and bright. This radius-albedo […]