Results 1 to 10 of about 252 (123)

Evidence for Water in the Rocky Debris of a Disrupted Extrasolar Minor Planet [PDF]

open access: yesScience, 2013
Remnants of a Water-Bearing World Stars like the Sun end their lives as white dwarfs. Farihi et al. (p. 218 ) used detailed spectroscopic analysis of a debris-accreting white dwarf, along with knowledge that such systems accrete this debris ...
J. Farihi, B. T. Gansicke, D. Koester
openaire   +3 more sources

CHEMICAL ABUNDANCES IN THE EXTERNALLY POLLUTED WHITE DWARF GD 40: EVIDENCE OF A ROCKY EXTRASOLAR MINOR PLANET [PDF]

open access: yesThe Astrophysical Journal, 2010
We present Keck/HIRES data with model atmosphere analysis of the helium-dominated polluted white dwarf GD 40, in which we measure atmospheric abundances relative to helium of 9 elements: H, O, Mg, Si, Ca, Ti, Cr, Mn, and Fe. Apart from hydrogen whose association with the other contaminants is uncertain, this material most likely accreted from GD 40's ...
Klein, B.   +4 more
openaire   +2 more sources

Potential Atmospheric Compositions of TRAPPIST-1 c Constrained by JWST/MIRI Observations at 15 μm

open access: yesThe Astrophysical Journal Letters, 2023
The first James Webb Space Telescope observations of TRAPPIST-1 c showed a secondary eclipse depth of 421 ± 94 ppm at 15 μ m, which is consistent with a bare rock surface or a thin, O _2 -dominated, low-CO _2 atmosphere. Here we further explore potential
Andrew P. Lincowski   +15 more
doaj   +1 more source

The Carbon-deficient Evolution of TRAPPIST-1c

open access: yesThe Astrophysical Journal, 2023
Transiting planets orbiting M dwarfs provide the best opportunity to study the atmospheres of rocky planets with current facilities. As JWST enters its second year of science operations, an important initial endeavor is to determine whether these rocky ...
Katie E. Teixeira   +3 more
doaj   +1 more source

Alternative Methylated Biosignatures. I. Methyl Bromide, a Capstone Biosignature

open access: yesThe Astrophysical Journal, 2022
The first potential exoplanetary biosignature detections are likely to be ambiguous due to the potential for false positives: abiotic planetary processes that produce observables similar to those anticipated from a global biosphere.
Michaela Leung   +3 more
doaj   +1 more source

Measuring the Obliquities of the TRAPPIST-1 Planets with MAROON-X

open access: yesThe Astronomical Journal, 2023
A star’s obliquity with respect to its planetary system can provide us with insight into the system’s formation and evolution, as well as hinting at the presence of additional objects in the system. However, M dwarfs, which are the most promising targets
Madison Brady   +8 more
doaj   +1 more source

Revising Properties of Planet–Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems

open access: yesThe Astronomical Journal, 2023
Binary stars are ubiquitous; the majority of solar-type stars exist in binaries. Exoplanet occurrence rate is suppressed in binaries, but some multiples do still host planets.
Kendall Sullivan   +9 more
doaj   +1 more source

Characterization of a Set of Small Planets with TESS and CHEOPS and an Analysis of Photometric Performance

open access: yesThe Astronomical Journal, 2023
The radius valley carries implications for how the atmospheres of small planets form and evolve, but this feature is visible only with highly precise characterizations of many small planets.
Dominic Oddo   +43 more
doaj   +1 more source

The Direct Mid-infrared Detectability of Habitable-zone Exoplanets around Nearby Stars

open access: yesThe Astronomical Journal, 2023
Giant planets within the habitable zones of the closest several stars can currently be imaged with ground-based telescopes. Within the next decade, the Extremely Large Telescopes (ELTs) will begin to image the habitable zones of a greater number of ...
Zach Werber, Kevin Wagner, Dániel Apai
doaj   +1 more source

Detecting Solar System Analogs through Joint Radial Velocity/Astrometric Surveys

open access: yesThe Astronomical Journal, 2023
Earth-mass exoplanets on year-long orbits and cool gas giants (CGG) on decade-long orbits lie at the edge of current detection limits. The Terra Hunting Experiment (THE) will take nightly radial velocity (RV) observations on HARPS3 of at least 40 bright ...
Daniel A. Yahalomi   +3 more
doaj   +1 more source

Home - About - Disclaimer - Privacy