Search Results - "Cruikshank, D.P"

Origin of the Pluto–Charon system: Constraints from the New Horizons flyby by McKinnon, William B., Stern, S.A., Weaver, H.A., Nimmo, F., Bierson, C.J., Grundy, W.M., Cook, J.C., Cruikshank, D.P., Parker, A.H., Moore, J.M., Spencer, J.R., Young, L.A., Olkin, C.B., Ennico Smith, K.

“…•Pluto and Charon are rock rich while the small satellites are mostly water ice.•Charon is about 10% icier than Pluto.•A giant impact origin involving…”
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Physical state and distribution of materials at the surface of Pluto from New Horizons LEISA imaging spectrometer by Schmitt, B., Philippe, S., Grundy, W.M., Reuter, D.C., Côte, R., Quirico, E., Protopapa, S., Young, L.A., Binzel, R.P., Cook, J.C., Cruikshank, D.P., Dalle Ore, C.M., Earle, A.M., Ennico, K., Howett, C.J.A., Jennings, D.E., Linscott, I.R., Lunsford, A.W., Olkin, C.B., Parker, A.H., Parker, J.Wm, Singer, K.N., Spencer, J.R., Stansberry, J.A., Stern, S.A., Tsang, C.C.C., Verbiscer, A.J., Weaver, H.A.

“…•The analysis of the first couple of LEISA/New Horizons spectro-images is performed.•Qualitative distribution maps are obtained for N2, CH4, CO, H2O and the…”
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The composition of “ultra-red” TNOs and centaurs by Dalle Ore, C. Morea, Barucci, M.A., Emery, J.P., Cruikshank, D.P., de Bergh, C., Roush, T.L., Perna, D., Merlin, F., Dalle Ore, L.V.

“…•We present composition predictions for faint TNOs and centaurs.•We analyze ten ultra-red objects making use of photometric data from 0.4 to 4.5μm.•We find…”
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Pluto's Sputnik Planitia: Composition of geological units from infrared spectroscopy by Scipioni, F., White, O., Cook, J.C., Bertrand, T., Cruikshank, D.P., Grundy, W.M., Beddingfield-Cartwright, C., Binzel, R.P., Dalle Ore, C.M., Jennings, D., Moore, J.M., Olkin, C.B., Protopapa, S., Reuter, D.C., Schmitt, B., Singer, K.N., Spencer, J.R., Stern, S.A., Weaver, H.A., Verbiscer, A.J., Young, L.A.

“…We have compared spectroscopic data of Sputnik Planitia on Pluto, as acquired by New Horizons' Linear Etalon Imaging Spectral Array (LEISA) instrument, to the…”
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Methane distribution on Pluto as mapped by the New Horizons Ralph/MVIC instrument by Earle, Alissa M., Grundy, W., Howett, C.J.A., Olkin, C.B., Parker, A.H., Scipioni, F., Binzel, R.P., Beyer, R.A., Cook, J.C., Cruikshank, D.P., Dalle Ore, C.M., Ennico, K., Protopapa, S., Reuter, D.C., Schenk, P.M., Schmitt, B., Stern, S.A., Weaver, H.A., Young, L.A.

“…•Presents maps of methane equivalent width (of the 890 nm band) and spectral slope based on data from the New Horizons Ralph/MVIC instrument.•Plutoś surface…”
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Distribution of icy particles across Enceladus' surface as derived from Cassini-VIMS measurements by Jaumann, R., Stephan, K., Hansen, G.B., Clark, R.N., Buratti, B.J., Brown, R.H., Baines, K.H., Newman, S.F., Bellucci, G., Filacchione, G., Coradini, A., Cruikshank, D.P., Griffith, C.A., Hibbitts, C.A., McCord, T.B., Nelson, R.M., Nicholson, P.D., Sotin, C., Wagner, R.

“…The surface of Enceladus consists almost completely of water ice. As the band depths of water ice absorptions are sensitive to the size of particles,…”
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Infrared (0.83–5.1 μm) photometry of Phoebe from the Cassini Visual Infrared Mapping Spectrometer by Buratti, B.J., Soderlund, K., Bauer, J., Mosher, J.A., Hicks, M.D., Simonelli, D.P., Jaumann, R., Clark, R.N., Brown, R.H., Cruikshank, D.P., Momary, T.

“…Three weeks prior to the commencement of Cassini's 4 year tour of the saturnian system, the spacecraft executed a close flyby of the outer satellite Phoebe…”
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Surface composition of Pluto's Kiladze area and relationship to cryovolcanism by Emran, A., Dalle Ore, C.M., Cruikshank, D.P., Cook, J.C.

“…A link between exposures of water (H2O) ice with traces of an ammoniated compound (e.g., a salt) and the probable effusion of a water-rich cryolava onto the…”
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Photometric properties of Titan's surface from Cassini VIMS: Relevance to titan's hemispherical albedo dichotomy and surface stability by Nelson, R.M., Brown, R.H., Hapke, B.W., Smythe, W.D., Kamp, L., Boryta, M.D., Leader, F., Baines, K.H., Bellucci, G., Bibring, J.-P., Buratti, B.J., Capaccioni, F., Cerroni, P., Clark, R.N., Combes, M., Coradini, A., Cruikshank, D.P., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D.L., McCord, T.B., Mennella, V., Nicholson, P.D., Sicardy, B., Sotin, C.

“…The Visual and Infrared Mapping Spectrometer (VIMS) instrument on the Cassini Saturn Orbiter returned spectral imaging data as the spacecraft undertook six…”
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Pluto’s global surface composition through pixel-by-pixel Hapke modeling of New Horizons Ralph/LEISA data by Protopapa, S., Grundy, W.M., Reuter, D.C., Hamilton, D.P., Dalle Ore, C.M., Cook, J.C., Cruikshank, D.P., Schmitt, B., Philippe, S., Quirico, E., Binzel, R.P., Earle, A.M., Ennico, K., Howett, C.J.A., Lunsford, A.W., Olkin, C.B., Parker, A., Singer, K.N., Stern, A., Verbiscer, A.J., Weaver, H.A., Young, L.A.

“…•Pixel-by-pixel Hapke modeling of New Horizons Ralph/LEISA data.•Maps of Pluto’s volatiles and non-volatiles components.•Latitudinal variations of CH4 and N2…”
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On the origin & thermal stability of Arrokoth's and Pluto's ices by Lisse, C.M., Young, L.A., Cruikshank, D.P., Sandford, S.A., Schmitt, B., Stern, S.A., Weaver, H.A., Umurhan, O., Pendleton, Y.J., Keane, J.T., Gladstone, G.R., Parker, J.M., Binzel, R.P., Earle, A.M., Horanyi, M., El-Maarry, M.R., Cheng, A.F., Moore, J.M., McKinnon, W.B., Grundy, W.M., Kavelaars, J.J., Linscott, I.R., Lyra, W., Lewis, B.L., Britt, D.T., Spencer, J.R., Olkin, C.B., McNutt, R.L., Elliott, H.A., Dello-Russo, N., Steckloff, J.K., Neveu, M., Mousis, O.

“…In this paper we discuss in a thermodynamic, geologically empirical way the long-term nature of the stable majority ices that could be present in Kuiper Belt…”
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Ices on Charon: Distribution of H2O and NH3 from New Horizons LEISA observations by Dalle Ore, C. Morea, Protopapa, S., Cook, J.C., Grundy, W.M., Cruikshank, D.P., Verbiscer, A.J., Ennico, K., Olkin, C.B., Stern, S.A., Weaver, H.A., Young, L.A.

“…•We map the composition of Charon surface from New Horizons LEISA data.•We present a map of the distribution of NH3 in H2O products on the surface of…”
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The CH4 cycles on Pluto over seasonal and astronomical timescales by Bertrand, T., Forget, F., Umurhan, O.M., Moore, J.M., Young, L.A., Protopapa, S., Grundy, W.M., Schmitt, B., Dhingra, R.D., Binzel, R.P., Earle, A.M., Cruikshank, D.P., Stern, S.A., Weaver, H.A., Ennico, K., Olkin, C.B.

“…Pluto's surface is covered in numerous CH4 ice deposits, that vary in texture and brightness, as revealed by the New Horizons spacecraft as it flew by Pluto in…”
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The CH 4 cycles on Pluto over seasonal and astronomical timescales by Bertrand, Tanguy, Forget, F., Umurhan, O.M. M, Moore, J.M. M, Young, L.A. A, Protopapa, S., Grundy, W.M. M, Schmitt, B., Dhingra, R.D. D, Binzel, R.P. P, Earle, A.M. M, Cruikshank, D.P. P, Stern, S.A. A, Weaver, H.A. A, Ennico, K., Olkin, C.B. B, Beyer, David P, O'Brien, Paul, Withers, Gwen

“…These observations suggest that CH 4 on Pluto has a complex history, involving reservoirs of different composition, thickness and stability controlled by…”
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Volatile transport modeling on Triton with new observational constraints by Bertrand, T., Lellouch, E., Holler, B.J., Young, L.A., Schmitt, B., Marques Oliveira, J., Sicardy, B., Forget, F., Grundy, W.M., Merlin, F., Vangvichith, M., Millour, E., Schenk, P.M., Hansen, C.J., White, O.L., Moore, J.M., Stansberry, J.A., Oza, A.V., Dubois, D., Quirico, E., Cruikshank, D.P.

“…Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of…”
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The surface compositions of Pluto and Charon by Cruikshank, D.P., Grundy, W.M., DeMeo, F.E., Buie, M.W., Binzel, R.P., Jennings, D.E., Olkin, C.B., Parker, J.W., Reuter, D.C., Spencer, J.R., Stern, S.A., Young, L.A., Weaver, H.A.

“…•Pluto’s surface is covered by CH4, N2, and CO ices, plus a non-ice component.•The distribution of Pluto’s ices is heterogeneous and time-variable.•The non-ice…”
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On the origin & thermal stability of Arrokoth's and Pluto's ice by C.M.Lisse, C.M.Lisse, L.A.Young, L.A.Young, Cruikshank, D.P., Sandford, S.A., B.Schmitt, B.Schmitt, Stern, S.A., Weaver, H.A., O.Umurhan, O.Umurhan, Y.J.Pendleton, Y.J.Pendleton, J.T.Keane, J.T.Keane, G.R.Gladstone, G.R.Gladstone, J.M.Parker, J.M.Parker, R.P.Binzel, R.P.Binzel, A.M.Earle, A.M.Earle, M.Horanyi, M.Horanyi, M.R.El-Maarry, M.R.El-Maarry, A.F.Cheng, A.F.Cheng, J.M.Moore, J.M.Moore, W.B.McKinnon, W.B.McKinnon, W.M.Grundy, W.M.Grundy, J.J.Kavelaars, J.J.Kavelaars, I.R.Linscott, I.R.Linscott, W.Lyra, W.Lyra, B.L.Lewis, B.L.Lewis, D.T.Britt, D.T.Britt, J.R.Spencer, J.R.Spencer, C.B.Olkin, C.B.Olkin, R.L.McNutt, R.L.McNutt, H.A.Elliott, H.A.Elliott, N.Dello-Russo, N.Dello-Russo, M.Neveu, M.Neveu, O.Mousis, O.Mousis

“…In this paper we discuss in a thermodynamic, geologically empirical way the long-term nature of the stable majority ices that could be present in Kuiper Belt…”
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Thermal emission spectroscopy (5.2–38 μm) of three Trojan asteroids with the Spitzer Space Telescope: Detection of fine-grained silicates by Emery, J.P., Cruikshank, D.P., Van Cleve, J.

“…We present thermal emission spectra (5.2–38 μm) of the Trojan asteroids 624 Hektor, 911 Agamemnon, and 1172 Aneas. The observations used the Infrared…”
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Multiple asteroid systems: Dimensions and thermal properties from Spitzer Space Telescope and ground-based observations by Marchis, F., Enriquez, J.E., Emery, J.P., Mueller, M., Baek, M., Pollock, J., Assafin, M., Vieira Martins, R., Berthier, J., Vachier, F., Cruikshank, D.P., Lim, L.F., Reichart, D.E., Ivarsen, K.M., Haislip, J.B., LaCluyze, A.P.

“…► Mid-IR spectra from 5.2 to 38μm using the Spitzer/IRS of 28 asteroids. ► Analyzed using STM and a thermophysical model (TPM) if 3D-shape is available. ►…”
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Hapke modeling of Rhea surface properties through Cassini-VIMS spectra by Ciarniello, M., Capaccioni, F., Filacchione, G., Clark, R.N., Cruikshank, D.P., Cerroni, P., Coradini, A., Brown, R.H., Buratti, B.J., Tosi, F., Stephan, K.

“…► Rhea’s spectrum and phase function modeling. ► Spectra from VIMS on board Cassini spacecraft. ► Intraparticle mixture of water ice and Triton tholin…”
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