Search Publications

The haze and methane distributions on Neptune from HST-STIS spectroscopy
DOI: 10.1016/j.icarus.2010.08.013 Bibcode: 2011Icar..211..780K

Karkoschka, Erich; Tomasko, Martin G.

We analyzed a data cube of Neptune acquired with the Hubble STIS spectrograph on August 3, 2003. The data covered the full afternoon hemisphere at 0.1 arcsec spatial resolution between 300 and 1000 nm wavelength at 1 nm resolution. Navigation was accurate to 0.004 arcsec and 0.05 nm. We constrained the vertical aerosol structure with radiative tra…

2011 Icarus
eHST 118
Methane on Uranus: The case for a compact CH 4 cloud layer at low latitudes and a severe CH 4 depletion at high-latitudes based on re-analysis of Voyager occultation measurements and STIS spectroscopy
DOI: 10.1016/j.icarus.2011.06.024 Bibcode: 2011Icar..215..292S

Sromovsky, L. A.; Fry, P. M.; Kim, J. H.

Lindal et al. (Lindal, G.F., Lyons, J.R., Sweetnam, D.N., Eshleman, V.R., Hinson, D.P. [1987]. J. Geophys. Res. 92 (11), 14987-15001) presented a range of temperature and methane profiles for Uranus that were consistent with 1986 Voyager radio occultation measurements of refractivity versus altitude. A localized refractivity slope variation near 1…

2011 Icarus
eHST 92
Saturn's zonal wind profile in 2004-2009 from Cassini ISS images and its long-term variability
DOI: 10.1016/j.icarus.2011.07.005 Bibcode: 2011Icar..215...62G

Hueso, R.; Sánchez-Lavega, A.; García-Melendo, E. +1 more

Five years of Cassini Imaging Science Subsystem images, from 2004 to 2009, are analyzed in this work to retrieve global zonal wind profiles of Saturn's northern and southern hemispheres in the methane absorbing bands at 890 and 727 nm and in their respective adjacent continuum wavelengths of 939 and 752 nm. A complete view of Saturn's global circu…

2011 Icarus
Cassini eHST 89
Five new and three improved mutual orbits of transneptunian binaries
DOI: 10.1016/j.icarus.2011.03.012 Bibcode: 2011Icar..213..678G

Buie, M. W.; Roe, H. G.; Nimmo, F. +7 more

We present three improved and five new mutual orbits of transneptunian binary systems (58534) Logos-Zoe, (66652) Borasisi-Pabu, (88611) Teharonhiawako-Sawiskera, (123509) 2000 WK 183, (149780) Altjira, 2001 QY 297, 2003 QW 111, and 2003 QY 90 based on Hubble Space Telescope and Keck II laser guide star a…

2011 Icarus
eHST 66
Stardust-NExT, Deep Impact, and the accelerating spin of 9P/Tempel 1
DOI: 10.1016/j.icarus.2011.01.006 Bibcode: 2011Icar..213..345B

Licandro, Javier; Vincent, J. -B.; Bhatt, B. C. +68 more

The evolution of the spin rate of Comet 9P/Tempel 1 through two perihelion passages (in 2000 and 2005) is determined from 1922 Earth-based observations taken over a period of 13 year as part of a World-Wide observing campaign and from 2888 observations taken over a period of 50 days from the Deep Impact spacecraft. We determine the following sider…

2011 Icarus
eHST 54
Vertical structure of Jupiter's Oval BA before and after it reddened: What changed?
DOI: 10.1016/j.icarus.2011.06.032 Bibcode: 2011Icar..215..211W

de Pater, Imke; Wong, Michael H.; Marcus, Philip S. +2 more

To constrain the properties of Oval BA before and after it reddened, we use Hubble methane band images from 1994 to 2009 to find that the distribution of upper tropospheric haze atop the oval and its progenitors remained unchanged, with reflectivity variations of less than 10% over this time span. We quantify measurement uncertainties and short-te…

2011 Icarus
eHST 36
Changes in Jupiter’s zonal velocity between 1979 and 2008
DOI: 10.1016/j.icarus.2010.11.018 Bibcode: 2011Icar..211.1215A

de Pater, Imke; Wong, Michael H.; Marcus, Philip S. +1 more

We show that the peak velocity of Jupiter's visible-cloud-level zonal winds near 24°N (planetographic) increased from 2000 to 2008. This increase was the only change in the zonal velocity from 2000 to 2008 for latitudes between ±70° that was statistically significant and not obviously associated with visible weather. We present the first automated…

2011 Icarus
eHST 36
Neptune's rotational period suggested by the extraordinary stability of two features
DOI: 10.1016/j.icarus.2011.05.013 Bibcode: 2011Icar..215..439K

Karkoschka, Erich

The interior rotation and motions in giant planets have generally been probed only at radio wavelengths from spacecraft near the planet, except for Jupiter's radio emission detectable from Earth. Here I suggest that Neptune's interior can be indirectly probed at visible wavelength by tracking 10 features that are connected with a stationary latitu…

2011 Icarus
eHST 33
Optical and infrared colors of transneptunian objects observed with HST
DOI: 10.1016/j.icarus.2011.03.005 Bibcode: 2011Icar..213..693B

Grundy, W. M.; Noll, K. S.; Benecchi, S. D. +2 more

We present optical colors of 72 transneptunian objects (TNOs), and infrared colors of 80 TNOs obtained with the WFPC2 and NICMOS instruments, respectively, on the Hubble Space Telescope (HST). Both optical and infrared colors are available for 32 objects that overlap between the datasets. This dataset adds an especially uniform, consistent and lar…

2011 Icarus
eHST 31
Photometry of Triton 1992-2004: Surface volatile transport and discovery of a remarkable opposition surge
DOI: 10.1016/j.icarus.2011.01.012 Bibcode: 2011Icar..212..835B

Buratti, B. J.; Hillier, J. K.; Hicks, M. D. +9 more

Triton, the large satellite of Neptune, was imaged by the Voyager 2 spacecraft in 1989 with dark plumes originating in its volatile-rich south polar region. Southern summer solstice, a time when seasonal volatile transport should be at a maximum, occurred in 2001. Ground-based observations of Triton's rotational light curve obtained from Table Mou…

2011 Icarus
eHST 31