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Keck near-infrared images of Neptune from UT 26 July 2007 show that the cloud feature typically observed within a few degrees of Neptune's south pole had split into a pair of bright spots. A careful determination of disk center places the…

地球与行星天体物理 · 物理学 2015-05-18 S. H. Luszcz-Cook , I. de Pater , M. Adamkovics , H. B. Hammel

A stellar occultation occurs when a Solar System object passes in front of a star for an observer. This technique allows the determination of sizes and shapes of the occulting body with kilometer precision. Also, this technique constrains…

The TRAPPIST-1 system is home to at least seven terrestrial planets and is a target of interest for future James Webb Space Telescope (JWST) observations. Additionally, these planets will be of interest to future missions making…

地球与行星天体物理 · 物理学 2022-07-26 Kathleen Mandt , Adrienn Luspay-Kuti , Jacob Lustig-Yaeger , Ryan Felton , Shawn Domagal-Goldman

A time-variable 1D photochemical model is used to study the distribution of stratospheric hydrocarbons as a function of altitude, latitude, and season on Uranus and Neptune. The results for Neptune indicate that in the absence of…

地球与行星天体物理 · 物理学 2018-03-29 Julianne I. Moses , Leigh N. Fletcher , Thomas K. Greathouse , Glenn S. Orton , Vincent Hue

We present new measurements of the vertical density profile of the Earth's atmosphere at altitudes between 70 and 200 km, based on Earth occultations of the Crab Nebula observed with the X-ray Imaging Spectrometer onboard Suzaku and the…

Technique: We present a method to determine the pressure at which significant cloud opacity is present between 2 and 6 bars on Jupiter. We use: a) the strength of a Fraunhofer absorption line in a zone to determine the ratio of reflected…

地球与行星天体物理 · 物理学 2015-09-23 G. L. Bjoraker , M. H. Wong , I. de Pater , M. Ádámkovics

Over the last decade there has been mounting evidence that the strength of the Sun's polar magnetic fields during a solar cycle minimum is the best predictor of the amplitude of the next solar cycle. Surface flux transport models can be…

太阳与恒星天体物理 · 物理学 2018-10-31 Lisa A. Upton , David H. Hathaway

The New Horizons spacecraft, which flew by Pluto on July 14, 2015, revealed the presence of haze in Pluto's atmosphere that were formed by CH4/N2 photochemistry at high altitudes in Pluto's atmosphere, as on Titan and Triton. In order to…

地球与行星天体物理 · 物理学 2017-03-08 Tanguy Bertrand , François Forget

Observations of Pluto's companion planet Charon have so far yielded no compelling evidence for a persistent atmosphere. However, with the upcoming encounter of New Horizons at the Pluto-Charon system, sensitivity to detection of a possible…

地球与行星天体物理 · 物理学 2016-05-31 Joshua A. Kammer , S. Alan Stern

We examine Saturn's atmosphere with observations from ground-based telescopes and Hubble Space Telescope (HST). We present a detailed analysis of observations acquired during 2018. A system of polar storms that appeared in the planet in…

Results are presented from a 3-D Pluto general circulation model (GCM) that includes conductive heating and cooling, non-local thermodynamic equilibrium (non-LTE) heating by methane at 2.3 and 3.3 microns, non-LTE cooling by cooling by…

地球与行星天体物理 · 物理学 2016-03-29 Angela M. Zalucha

Recently discovered exoplanets on close-in orbits should have surface temperatures of 100's to 1000's of K. They are likely tidally locked and synchronously rotating around their parent stars and, if an atmosphere is absent, have surface…

地球与行星天体物理 · 物理学 2015-05-28 Joost van Summeren , Clinton P. Conrad , Eric Gaidos

Between 2001 and 2023, we obtained high spectral resolution mid-infrared observations of Io using the TEXES instrument at NASA's Infrared Telescope Facility. These observations were centered at 529.8 cm-1 (18.88 {\mu}m) and include several…

From 1988 to 2016, several stellar occultations have been observed to characterize Pluto's atmosphere and its evolution (Meza et al, 2019). From each stellar occultation, an accurate astrometric position of Pluto at the observation epoch is…

We investigate how night side cooling and surface friction impact surface temperatures and large scale circulation for tidally locked Earth-like planets. For each scenario, we vary the orbital period between $P_{rot}=1-100$~days and capture…

地球与行星天体物理 · 物理学 2016-06-01 L. Carone , R. Keppens , L. Decin

The nature of the flow below the cloud level on Jupiter and Saturn is still unknown. Relating the flow on these planets to perturbations in their density field is key to the analysis of the gravity measurements expected from both the Juno…

地球与行星天体物理 · 物理学 2016-12-21 Eli Galanti , Yohai Kaspi , Eli Tziperman

The NASA New Horizons spacecraft flies past Pluto on July 14, 2015, carrying two instruments that detect charged particles. Pluto has a tenuous, extended atmosphere that is escaping the weak gravity of the planet. The interaction of the…

The orbit of the outer satellite Alexhelios of (216) Kleopatra is already constrained by adaptive-optics astrometry, obtained with the VLT/SPHERE instrument. However, there is also a preceding occultation event in 1980 attributed to this…

地球与行星天体物理 · 物理学 2022-01-19 M. Brož , J. Ďurech , B. Carry , F. Vachier , F. Marchis , J. Hanuš , L. Jorda , P. Vernazza , D. Vokrouhlický , M. Walterová , R. Behrend