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of 6
pro vyhledávání: '"Noah W. Tuchow"'
Publikováno v:
The Astronomical Journal, Vol 167, Iss 3, p 139 (2024)
The Habitable Worlds Observatory Preliminary Input Catalog (HPIC) is a list of ∼13,000 nearby bright stars that will be potential targets for the Habitable Worlds Observatory (HWO) in its search for Earth-sized planets around Sun-like stars. We con
Externí odkaz:
https://doaj.org/article/10f755a610eb45aa926b1033ac165a31
Autor:
Noah W. Tuchow, Jason T. Wright
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 1, p 71 (2023)
A planet’s history dictates its current potential to host habitable conditions and life. The concept of the continuously habitable zone (CHZ) has been used to define the region around a star most likely to host planets with long-term habitability.
Externí odkaz:
https://doaj.org/article/9a532503a5a24779b4446503feae03f3
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 484:3772-3784
Transit timing variations (TTVs) are a valuable tool to determine the masses and orbits of transiting planets in multi-planet systems. TTVs can be readily modeled given knowledge of the interacting planets’ orbital configurations and planet-star ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::23add015b6367080f1930391f2687904
https://doi.org/10.1093/mnras/stz247
https://doi.org/10.1093/mnras/stz247
Autor:
Noah W. Tuchow, Jason T. Wright
Future exoplanet direct imaging missions, such as HabEx and LUVOIR, will select target stars to maximize the number of Earth-like exoplanets that can have their atmospheric compositions characterized. Because one of these missions’ aims is to detec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ea446298b76d98428c2132f96af361d
Autor:
Jason T. Wright, Noah W. Tuchow
Publikováno v:
Research Notes of the AAS. 5:194
Stars do not remain static, so their habitable zones evolve in time. Over a star's evolution, its habitable zone encompasses new planets, and it remains uncertain whether these planets can become habitable. We refer to this often overlooked class of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::80510480769178406dd1fe12177455ee
https://doi.org/10.3847/2515-5172/ac1ea2
https://doi.org/10.3847/2515-5172/ac1ea2
Publikováno v:
Optics Express. 24:18559
To solve the radiative transfer equation and relate inherent optical properties (IOPs) to apparent optical properties (AOPs), knowledge of the volume scattering phase function is required. Due to the difficulty of measuring the phase function, it is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd20e728bc06add3d0fce215d39a01fb
https://doi.org/10.1364/oe.24.018559
https://doi.org/10.1364/oe.24.018559