Exoplanet clouds
C Helling - Annual Review of Earth and Planetary Sciences, 2019 - annualreviews.org
Clouds, which are common features in Earth's atmosphere, form in atmospheres of planets
that orbit other stars than our Sun, in so-called extrasolar planets or exoplanets. Exoplanet …
that orbit other stars than our Sun, in so-called extrasolar planets or exoplanets. Exoplanet …
Clouds and hazes in exoplanet atmospheres
Clouds and hazes are commonplace in the atmospheres of solar system planets and are
likely ubiquitous in the atmospheres of extrasolar planets as well. Clouds affect every aspect …
likely ubiquitous in the atmospheres of extrasolar planets as well. Clouds affect every aspect …
A new set of atmosphere and evolution models for cool T–Y brown dwarfs and giant exoplanets
We present a new set of solar metallicity atmosphere and evolutionary models for very cool
brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere …
brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere …
The transit light source effect: false spectral features and incorrect densities for M-dwarf transiting planets
BV Rackham, D Apai, MS Giampapa - The Astrophysical Journal, 2018 - iopscience.iop.org
Transmission spectra are differential measurements that utilize stellar illumination to probe
transiting exoplanet atmospheres. Any spectral difference between the illuminating light …
transiting exoplanet atmospheres. Any spectral difference between the illuminating light …
Constraining the Nature of the PDS 70 Protoplanets with VLTI/GRAVITY∗
We present K-band interferometric observations of the PDS 70 protoplanets along with their
host star using VLTI/GRAVITY. We obtained K-band spectra and 100 μas precision …
host star using VLTI/GRAVITY. We obtained K-band spectra and 100 μas precision …
Direct confirmation of the radial-velocity planet β Pictoris c
M Nowak, S Lacour, AM Lagrange, P Rubini… - Astronomy & …, 2020 - aanda.org
Context. Methods used to detect giant exoplanets can be broadly divided into two
categories: indirect and direct. Indirect methods are more sensitive to planets with a small …
categories: indirect and direct. Indirect methods are more sensitive to planets with a small …
Aerosols in exoplanet atmospheres
Observations of exoplanet atmospheres have shown that aerosols, like in the solar system,
are common across a variety of temperatures and planet types. The formation and …
are common across a variety of temperatures and planet types. The formation and …
The prevalence of dust on the exoplanet HD 189733b from Hubble and Spitzer observations
The hot Jupiter HD 189733b is the most extensively observed exoplanet. Its atmosphere has
been detected and characterized in transmission and eclipse spectroscopy, and its phase …
been detected and characterized in transmission and eclipse spectroscopy, and its phase …
Peering into the formation history of β Pictoris b with VLTI/GRAVITY long-baseline interferometry
M Nowak, S Lacour, P Mollière, J Wang… - Astronomy & …, 2020 - aanda.org
Context. β Pictoris is arguably one of the most studied stellar systems outside of our own.
Some 30 yr of observations have revealed a highly-structured circumstellar disk, with rings …
Some 30 yr of observations have revealed a highly-structured circumstellar disk, with rings …
Simulations of stellar convection with CO5BOLD
B Freytag, M Steffen, HG Ludwig… - Journal of …, 2012 - Elsevier
High-resolution images of the solar surface show a granulation pattern of hot rising and
cooler downward-sinking material–the top of the deep-reaching solar convection zone …
cooler downward-sinking material–the top of the deep-reaching solar convection zone …