Zobrazeno 1 - 10
of 2 700
pro vyhledávání: '"Marley, M S"'
Autor:
Boehm, V. A., Lewis, N. K., Fairman, C. E., Moran, S. E., Gascón, C., Wakeford, H. R., Alam, M. K., Alderson, L., Barstow, J., Batalha, N. E., Grant, D., López-Morales, M., MacDonald, R. J., Marley, M. S., Ohno, K.
Ultraviolet wavelengths offer unique insights into aerosols in exoplanetary atmospheres. However, only a handful of exoplanets have been observed in the ultraviolet to date. Here, we present the ultraviolet-visible transmission spectrum of the inflat
Externí odkaz:
http://arxiv.org/abs/2410.17368
Autor:
Fortney, J. J., Militzer, B., Mankovich, C. R., Helled, R., Wahl, S. M., Nettelmann, N., Hubbard, W. B., Stevenson, D. J., Iess, L., Marley, M. S., Movshovitz, N.
We present a review of Saturn's interior structure and thermal evolution, with a particular focus on work in the past 5 years. Data from the Cassini mission, including a precise determination of the gravity field from the Grand Finale orbits, and the
Externí odkaz:
http://arxiv.org/abs/2304.09215
Autor:
Casewell, S. L., Debes, J., Braker, I. P., Cushing, M. C., Mace, G., Marley, M. S., Kirkpatrick, J. Davy
We present Spitzer observations at 3.6 and 4.5 microns and a near-infrared IRTF SpeX spectrum of the irradiated brown dwarf NLTT5306B. We determine that the brown dwarf has a spectral type of L5 and is likely inflated, despite the low effective tempe
Externí odkaz:
http://arxiv.org/abs/2010.07398
The reflected light signal from a planet throughout its orbit is a powerful probe of a planet's atmospheric properties. There are a number of planets that are amenable to reflected light phase curve studies with present and future space-based instrum
Externí odkaz:
http://arxiv.org/abs/1905.12662
Spectroscopic transiting observations of the atmospheres of hot Jupiters around other stars, first with Hubble Space Telescope and then Spitzer, opened the door to compositional studies of exoplanets. The James Webb Space Telescope will provide such
Externí odkaz:
http://arxiv.org/abs/1904.00054
Autor:
Casewell, S. L., Littlefair, S. P., Parsons, S. G., Marsh, T. R., Fortney, J. J., Marley, M. S.
We have observed the eclipsing, post-common envelope white dwarf-brown dwarf binary, SDSS141126.20+200911.1, in the near-IR with the HAWK-I imager, and present here the first direct detection of the dark side of an irradiated brown dwarf in the $H$ b
Externí odkaz:
http://arxiv.org/abs/1809.10205
Autor:
Lewis, N. K., Parmentier, V., Kataria, T., de Wit, J., Showman, A. P., Fortney, J. J., Marley, M. S.
Observations of the highly-eccentric (e~0.9) hot-Jupiter HD 80606b with Spitzer have provided some of best probes of the physics at work in exoplanet atmospheres. By observing HD 80606b during its periapse passage, atmospheric radiative, advective, a
Externí odkaz:
http://arxiv.org/abs/1706.00466
Autor:
Gaulme, P., Rowe, J. F., Bedding, T. R., Benomar, O., Corsaro, E., Davies, G. R., Hale, S. J., Howe, R., Garcia, R. A., Huber, D., Jiménez, A., Mathur, S., Mosser, B., Appourchaux, T., Boumier, P., Jackiewicz, J., Leibacher, J., Schmider, F. -X., Hammel, H. B., Lissauer, J. J., Marley, M. S., Simon, A. A., Chaplin, W. J., Elsworth, Y., Guzik, J. A., Murphy, N., Aguirre, V. Silva
Publikováno v:
The Astrophysical Journal Letters, Volume 833, Issue 1, article id. L13, 7 pp. (2016)
Starting in December 2014, Kepler K2 observed Neptune continuously for 49 days at a 1-minute cadence. The goals consisted of studying its atmospheric dynamics (Simon et al. 2016), detecting its global acoustic oscillations (Rowe et al., submitted), a
Externí odkaz:
http://arxiv.org/abs/1612.04287
Autor:
Mayorga, L. C., Jackiewicz, J., Rages, K., West, R. A., Knowles, B., Lewis, N., Marley, M. S.
We present phase curves of Jupiter from 0-140 degrees as measured in multiple optical bandpasses by Cassini/ISS during the Millennium flyby of Jupiter in late 2000 to early 2001. Phase curves are of interest for studying the energy balance of Jupiter
Externí odkaz:
http://arxiv.org/abs/1610.07679
Autor:
Moses, J. I., Marley, M. S., Zahnle, K., Line, M. R., Fortney, J. J., Barman, T. S., Visscher, C., Lewis, N. K., Wolff, M. J.
The past decade has seen significant progress on the direct detection and characterization of young, self-luminous giant planets at wide orbital separations from their host stars. Some of these planets show evidence for disequilibrium processes like
Externí odkaz:
http://arxiv.org/abs/1608.08643