A volcanically active planet is shown in closeup at the left side of the image with glowing eruptions and lines of lava on the surface. To the right and in the distance is a faint blue glowing ball representing the more massive planet in the system.Sixteen frames from Voyager 1's flyby of Jupiter in 1979 were merged to create this image. Jupiter's Great Red Spot is visible in the center. Jupiter's moon Europa can be seen in the foreground at the bottom left of the image.The frame is a horizontal rainbow of color on a grid. Shadows of molecules can be seen through the light as well as the jagged peaks and troughs of spectral lines.
Fizzy Super Earths and Lava Worlds“Fizzy Super-Earths: Impacts of Magma Composition on the Bulk Density and Structure of Lava Worlds.” in The Astrophysical Journal.01/03
Identifying Hydrothermal Activity on Icy Ocean Worlds“Ethene-ethanol ratios as potential indicators of hydrothermal activity at Enceladus, Europa, and other icy ocean worlds.” In Icarus.02/03
NASA Raman Spectroscopic Database"The NASA Raman spectroscopic database: Ramdb version 1.00.” In Icarus.03/03
NextPrevious
Go Explore
November 2013MEMS harsh environment sensor array-enabled hot spring mapping

Oiler, J., Shock, E., Hartnett, H., & Yu, H. (2013). 2013 IEEE SENSORS. doi:10.1109/icsens.2013.6688332

Lipidomics for Geochemistry

Pearson, A. (2014). Treatise on Geochemistry, None(None), 291–336. doi:10.1016/b978-0-08-095975-7.01022-6

Biofilm Growth and Fossil Form

Petroff, A. P., Beukes, N. J., Rothman, D. H., & Bosak, T. (2013). Physical Review X, 3(4), None. doi:10.1103/physrevx.3.041012

Warming early Mars with CO2 and H2

Ramirez, R. M., Kopparapu, R., Zugger, M. E., Robinson, T. D., Freedman, R., & Kasting, J. F. (2013). Nature Geosci, 7(1), 59–63. doi:10.1038/ngeo2000

Nitrogen solubility in molten metal and silicate at high pressure and temperature

Roskosz, M., Bouhifd, M. A., Jephcoat, A. P., Marty, B., & Mysen, B. O. (2013). Geochimica et Cosmochimica Acta, 121(None), 15–28. doi:10.1016/j.gca.2013.07.007

The HITRAN2012 molecular spectroscopic database

Rothman, L. S., Gordon, I. E., Babikov, Y., Barbe, A., Chris Benner, D., Bernath, P. F., … Birk, M. (2013). Journal of Quantitative Spectroscopy and Radiative Transfer, 130(None), 4–50. doi:10.1016/j.jqsrt.2013.07.002

Modeling of nitrogen compounds in cometary atmospheres: Fluorescence models of ammonia (NH3), hydrogen cyanide (HCN), hydrogen isocyanide (HNC) and cyanoacetylene (HC3N)

Villanueva, G. L., Magee-Sauer, K., & Mumma, M. J. (2013). Journal of Quantitative Spectroscopy and Radiative Transfer, 129(None), 158–168. doi:10.1016/j.jqsrt.2013.06.010

Activation and Proton Transport Mechanism in Influenza A M2 Channel

Wei, C., & Pohorille, A. (2013). Biophysical Journal, 105(9), 2036–2045. doi:10.1016/j.bpj.2013.08.030

WATER LOSS FROM TERRESTRIAL PLANETS WITH CO 2 -RICH ATMOSPHERES

Wordsworth, R. D., & Pierrehumbert, R. T. (2013). The Astrophysical Journal, 778(2), 154. doi:10.1088/0004-637x/778/2/154

Iron Isotope Characteristics of Hot Springs at Chocolate Pots, Yellowstone National Park

Wu, L., Brucker, R. P., Beard, B. L., Roden, E. E., & Johnson, C. M. (2013). Astrobiology, 13(11), 1091–1101. doi:10.1089/ast.2013.0996