Search Results - "Meadows, Victoria"
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Reflections on O 2 as a Biosignature in Exoplanetary Atmospheres
Published in Astrobiology (01-10-2017)“…Oxygenic photosynthesis is Earth's dominant metabolism, having evolved to harvest the largest expected energy source at the surface of most terrestrial…”
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Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides
Published in The planetary science journal (22-01-2021)“…We have collected transit times for the TRAPPIST-1 system with the Spitzer Space Telescope over four years. We add to these ground-based, HST, and K2…”
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Modeling Repeated M Dwarf Flaring at an Earth-like Planet in the Habitable Zone: Atmospheric Effects for an Unmagnetized Planet
Published in Astrobiology (01-01-2019)“…Understanding the impact of active M dwarf stars on the atmospheric equilibrium and surface conditions of a habitable zone Earth-like planet is key to…”
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Evolved Climates and Observational Discriminants for the TRAPPIST-1 Planetary System
Published in The Astrophysical journal (01-11-2018)“…The TRAPPIST-1 planetary system provides an unprecedented opportunity to study terrestrial exoplanet evolution with the James Webb Space Telescope (JWST) and…”
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Pale Orange Dots: The Impact of Organic Haze on the Habitability and Detectability of Earthlike Exoplanets
Published in The Astrophysical journal (10-02-2017)“…Hazes are common in known planetary atmospheres, and geochemical evidence suggests that early Earth occasionally supported an organic haze with significant…”
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THE EFFECTS OF REFRACTION ON TRANSIT TRANSMISSION SPECTROSCOPY: APPLICATION TO EARTH-LIKE EXOPLANETS
Published in The Astrophysical journal (01-09-2014)“…We quantify the effects of refraction in transit transmission spectroscopy on spectral absorption features and on temporal variations that could be used to…”
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The Pale Orange Dot: The Spectrum and Habitability of Hazy Archean Earth
Published in Astrobiology (01-11-2016)“…Recognizing whether a planet can support life is a primary goal of future exoplanet spectral characterization missions, but past research on habitability…”
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The effect of a strong stellar flare on the atmospheric chemistry of an earth-like planet orbiting an M dwarf
Published in Astrobiology (01-09-2010)“…Main sequence M stars pose an interesting problem for astrobiology: their abundance in our galaxy makes them likely targets in the hunt for habitable planets,…”
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THE EVOLUTION OF SOLAR FLUX FROM 0.1 nm TO 160 μm: QUANTITATIVE ESTIMATES FOR PLANETARY STUDIES
Published in The Astrophysical journal (20-09-2012)Get full text
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HAZMAT. V. The Ultraviolet and X-Ray Evolution of K Stars
Published in The Astrophysical journal (10-02-2019)“…Knowing the high-energy radiation environment of a star over a planet's formation and evolutionary period is critical in determining if that planet is…”
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Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment
Published in Astrobiology (01-06-2018)“…We describe how environmental context can help determine whether oxygen (O ) detected in extrasolar planetary observations is more likely to have a biological…”
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ABIOTIC OZONE AND OXYGEN IN ATMOSPHERES SIMILAR TO PREBIOTIC EARTH
Published in The Astrophysical journal (10-09-2014)“…The search for life on planets outside our solar system will use spectroscopic identification of atmospheric biosignatures. The most robust remotely detectable…”
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No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c
Published in Nature (London) (24-08-2023)“…Seven rocky planets orbit the nearby dwarf star TRAPPIST-1, providing a unique opportunity to search for atmospheres on small planets outside the Solar System…”
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THE INNER EDGE OF THE HABITABLE ZONE FOR SYNCHRONOUSLY ROTATING PLANETS AROUND LOW-MASS STARS USING GENERAL CIRCULATION MODELS
Published in The Astrophysical journal (01-03-2016)“…ABSTRACT Terrestrial planets at the inner edge of the habitable zone (HZ) of late-K and M-dwarf stars are expected to be in synchronous rotation, as a…”
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HAZMAT VI: The Evolution of Extreme Ultraviolet Radiation Emitted from Early M Stars
Published in The Astrophysical journal (01-05-2020)“…Quantifying the evolution of stellar extreme ultraviolet (EUV, 100-1000 ) emission is critical for assessing the evolution of planetary atmospheres and the…”
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Organic Haze as a Biosignature in Anoxic Earth-like Atmospheres
Published in Astrobiology (01-03-2018)“…Early Earth may have hosted a biologically mediated global organic haze during the Archean eon (3.8-2.5 billion years ago). This haze would have significantly…”
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Mitigating Worst-case Exozodiacal Dust Structure in High-contrast Images of Earth-like Exoplanets
Published in The Astronomical journal (01-11-2023)“…Detecting Earth-like exoplanets in direct images of nearby Sun-like systems brings a unique set of challenges that must be addressed in the early phases of…”
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Interferon-β Plays a Detrimental Role in Experimental Traumatic Brain Injury by Enhancing Neuroinflammation That Drives Chronic Neurodegeneration
Published in The Journal of neuroscience (11-03-2020)“…DNA damage and type I interferons (IFNs) contribute to inflammatory responses after traumatic brain injury (TBI). TBI-induced activation of microglia and…”
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Old age increases microglial senescence, exacerbates secondary neuroinflammation, and worsens neurological outcomes after acute traumatic brain injury in mice
Published in Neurobiology of aging (01-05-2019)“…After traumatic brain injury (TBI), individuals aged over 65 years show increased mortality and worse functional outcomes compared with younger persons. As…”
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HAZMAT. IV. Flares and Superflares on Young M Stars in the Far Ultraviolet
Published in The Astrophysical journal (01-11-2018)“…Abstract M stars are powerful emitters of far-ultraviolet light. Over long timescales, a significant, possibly dominant, fraction of this emission is produced…”
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