Zobrazeno 1 - 10
of 557
pro vyhledávání: '"Robinson, Tyler"'
Autor:
Morgan, Rhonda, Savransky, Dmitry, Turmon, Michael, Damiano, Mario, Hu, Renyu, Mennesson, Bertrand, Mamajek, Eric E., Robinson, Tyler D., Tokadjian, Armen
Publikováno v:
SPIE 130925M (2024)
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 microns an
Externí odkaz:
http://arxiv.org/abs/2410.16492
Microphysical Prescriptions for Parameterized Water Cloud Formation on Ultra-cool Substellar Objects
Publikováno v:
2024 ApJ 974 190
Water must condense into ice clouds in the coldest brown dwarfs and exoplanets. When they form, these icy clouds change the emergent spectra, temperature structure, and albedo of the substellar atmosphere. The properties of clouds are governed by com
Externí odkaz:
http://arxiv.org/abs/2408.08958
Survey strategies for upcoming exoplanet direct imaging missions have considered varying assumptions of prior knowledge. Precursor radial velocity surveys could have detected nearby exo-Earths and provided prior orbit and mass constraints. Alternativ
Externí odkaz:
http://arxiv.org/abs/2406.07749
Autor:
Stark, Christopher C., Mennesson, Bertrand, Bryson, Steve, Ford, Eric B., Robinson, Tyler D., Belikov, Ruslan, Bolcar, Matthew R., Feinberg, Lee D., Guyon, Olivier, Latouf, Natasha, Mandell, Avi M., Rauscher, Bernard J., Sirbu, Dan, Tuchow, Noah W.
The Habitable Worlds Observatory (HWO) will seek to detect and characterize potentially Earth-like planets around other stars. To ensure that the mission achieves the Astro2020 Decadal's recommended goal of 25 exoEarth candidates (EECs), we must take
Externí odkaz:
http://arxiv.org/abs/2405.19418
Autor:
Yang, Huanzhou, Komacek, Thaddeus D., Toon, Owen B., Wolf, Eric T., Robinson, Tyler D., Chael, Caroline, Abbot, Dorian S.
Publikováno v:
Huanzhou Yang et al 2024 ApJ 966 152
Potentially habitable exoplanets are targets of great interest for the James Webb Space Telescope and upcoming mission concepts such as the Habitable Worlds Observatory. Clouds strongly affect climate and habitability, but predicting their properties
Externí odkaz:
http://arxiv.org/abs/2405.03570
Autor:
Limbach, Mary Anne, Lustig-Yaeger, Jacob, Vanderburg, Andrew, Vos, Johanna M., Heller, Rene, Robinson, Tyler D.
The highest priority recommendation of the Astro2020 Decadal Survey for space-based astronomy was the construction of an observatory capable of characterizing habitable worlds. In this paper series we explore the detectability of and interference fro
Externí odkaz:
http://arxiv.org/abs/2405.02408
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 similar to Earth
Externí odkaz:
http://arxiv.org/abs/2404.16126
Autor:
Strauss, Ryder H., Robinson, Tyler D., Trilling, David E., Cummings, Ryan, Smith, Christopher J.
Publikováno v:
AJ 167 87 (2024)
The Galileo spacecraft had distant encounters with Earth in 1990 and 1992. Limited Solid State Imager (SSI) data acquired during these encounters has been previously presented, but the majority of the data from these Earth flybys have not been presen
Externí odkaz:
http://arxiv.org/abs/2402.00984
Autor:
Windsor, James D., Robinson, Tyler D., Kopparapu, Ravi kumar, Salvador, Arnaud, Young, Amber V., Meadows, Victoria S.
Understanding the limits of rocky planet habitability is one of the key goals of current and future exoplanet characterization efforts. An intrinsic concept of rocky planet habitability is the Habitable Zone. To date, the most widely used estimates o
Externí odkaz:
http://arxiv.org/abs/2401.12204
Autor:
Hall, Sawyer, Krissansen-Totton, Joshua, Robinson, Tyler, Salvador, Arnaud, Fortney, Jonathan J.
Publikováno v:
The Astronomical Journal, 166, 254. (2023)
Direct imaging spectroscopy with future space-based telescopes will constrain terrestrial planet atmospheric composition and potentially detect biosignature gases. One promising indication of life is abundant atmospheric O2. However, various non-biol
Externí odkaz:
http://arxiv.org/abs/2311.13001