9 results on '"Kissel, Jochen"'
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2. EPOXI at Comet Hartley 2
- Author
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A'Hearn, Michael F., Belton, Michael J. S., Delamere, W. Alan, Feaga, Lori M., Hampton, Donald, Kissel, Jochen, Klaasen, Kenneth P., McFadden, Lucy A., Meech, Karen J., Melosh, H. Jay, Schultz, Peter H., Sunshine, Jessica M., Thomas, Peter C., Veverka, Joseph, Wellnitz, Dennis D., Yeomans, Donald K., Besse, Sebastien, Bodewits, Dennis, Bowling, Timothy J., Carcich, Brian T., Collins, Steven M., Farnham, Tony L., Groussin, Olivier, Hermalyn, Brendan, Kelley, Michael S., Li, Jian-Yang, Lindler, Don J., Lisse, Carey M., McLaughlin, Stephanie A., Merlin, Frédéric, Protopapa, Silvia, Richardson, James E., and Williams, Jade L.
- Published
- 2011
- Full Text
- View/download PDF
3. Impact Features on Stardust: Implications for Comet 81p/Wild 2 Dust
- Author
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Hörz, Friedrich, Bastien, Ron, Borg, Janet, Bradley, John P., Bridges, John C., Brownlee, Donald E., Burchell, Mark J., Chi, Miaofang, Cintala, Mark J., Dai, Zu Rong, Djouadi, Zahia, Dominguez, Gerardo, Economou, Thanasis E., Fairey, Sam A. J., Floss, Christine, Franchi, Ian A., Graham, Giles A., Green, Simon F., Heck, Philipp, Hoppe, Peter, Huth, Joachim, Ishii, Hope, Kearsley, Anton T., Kissel, Jochen, Leitner, Jan, Leroux, Hugues, Marhas, Kuljeet, Messenger, Keiko, Schwandt, Craig S., See, Thomas H., Snead, Christopher, Stadermann, Frank J., Stephan, Thomas, Stroud, Rhonda, Teslich, Nick, Trigo-Rodríguez, Josep M., Tuzzolino, A. J., Troadec, David, Tsou, Peter, Warren, Jack, Westphal, Andrew, Wozniakiewicz, Penelope, Wright, Ian, and Zinner, Ernst
- Published
- 2006
- Full Text
- View/download PDF
4. Comet 81p/Wild 2 under a Microscope
- Author
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Brownlee, Don, Tsou, Peter, Aléon, Jérôme, Alexander, Conel M. O'D., Araki, Tohru, Bajt, Sasa, Baratta, Giuseppe A., Bastien, Ron, Bland, Phil, Bleuet, Pierre, Borg, Janet, Bradley, John P., Brearley, Adrian, Brenker, F., Brennan, Sean, Bridges, John C., Browning, Nigel D., Brucato, John R., Bullock, E., Burchell, Mark J., Busemann, Henner, Butterworth, Anna, Chaussidon, Marc, Cheuvront, Allan, Chi, Miaofang, Cintala, Mark J., Clark, B. C., Clemett, Simon J., Cody, George, Colangeli, Luigi, Cooper, George, Cordier, Patrick, Daghlian, C., Dai, Zurong, D'Hendecourt, Louis, Djouadi, Zahia, Dominguez, Gerardo, Duxbury, Tom, Dworkin, Jason P., Ebel, Denton S., Economou, Thanasis E., Fakra, Sirine, Fairey, Sam A. J., Fallon, Stewart, Ferrini, Gianluca, Ferroir, T., Fleckenstein, Holger, Floss, Christine, Flynn, George, Franchi, Ian A., Fries, Marc, Gainsforth, Z., Gallien, J.-P., Genge, Matt, Gilles, Mary K., Gillet, Philipe, Gilmour, Jamie, Glavin, Daniel P., Gounelle, Matthieu, Grady, Monica M., Graham, Giles A., Grant, P. G., Green, Simon F., Grossemy, Faustine, Grossman, Lawrence, Grossman, Jeffrey N., Guan, Yunbin, Hagiya, Kenji, Harvey, Ralph, Heck, Philipp, Herzog, Gregory F., Hoppe, Peter, Hörz, Friedrich, Huth, Joachim, Hutcheon, Ian D., Ignatyev, Konstantin, Ishii, Hope, Ito, Motoo, Jacob, Damien, Jacobsen, Chris, Jacobsen, Stein, Jones, Steven, Joswiak, David, Jurewicz, Amy, Kearsley, Anton T., Keller, Lindsay P., Khodja, H., Kilcoyne, A. L. David, Kissel, Jochen, Krot, Alexander, Langenhorst, Falko, Lanzirotti, Antonio, Le, Loan, Leshin, Laurie A., Leitner, J., Lemelle, L., Leroux, Hugues, Liu, Ming-Chang, Leuning, K., Lyon, Ian, MacPherson, Glen, Marcus, Matthew A., Marhas, Kuljeet, Marty, Bernard, Matrajt, Graciela, McKeegan, Kevin, Meibom, Anders, Mennella, Vito, Messenger, Keiko, Messenger, Scott, Mikouchi, Takeshi, Mostefaoui, Smail, Nakamura, Tomoki, Nakano, T., Newville, M., Nittler, Larry R., Ohnishi, Ichiro, Ohsumi, Kazumasa, Okudaira, Kyoko, Papanastassiou, Dimitri A., Palma, Russ, Palumbo, Maria E., Pepin, Robert O., Perkins, David, Perronnet, Murielle, Pianetta, P., Rao, William, Rietmeijer, Frans J. M., Robert, François, Rost, D., Rotundi, Alessandra, Ryan, Robert, Sandford, Scott A., Schwandt, Craig S., See, Thomas H., Schlutter, Dennis, Sheffield-Parker, J., Simionovici, Alexandre, Simon, Steven, Sitnitsky, I., Snead, Christopher J., Spencer, Maegan K., Stadermann, Frank J., Steele, Andrew, Stephan, Thomas, Stroud, Rhonda, Susini, Jean, Sutton, S. R., Suzuki, Y., Taheri, Mitra, Taylor, Susan, Teslich, Nick, Tomeoka, Kazu, Tomioka, Naotaka, Toppani, Alice, Trigo-Rodríguez, Josep M., Troadec, David, Tsuchiyama, Akira, Tuzzolino, Anthony J., Tyliszczak, Tolek, Uesugi, K., Velbel, Michael, Vellenga, Joe, Vicenzi, E., Vincze, L., Warren, Jack, Weber, Iris, Weisberg, Mike, Westphal, Andrew J., Wirick, Sue, Wooden, Diane, Wopenka, Brigitte, Wozniakiewicz, Penelope, Wright, Ian, Yabuta, Hikaru, Yano, Hajime, Young, Edward D., Zare, Richard N., Zega, Thomas, Ziegler, Karen, Zimmerman, Laurent, Zinner, Ernst, and Zolensky, Michael
- Published
- 2006
- Full Text
- View/download PDF
5. Surface of young Jupiter family Comet 81 P/Wild 2: view from the Stardust spacecraft
- Author
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Brownlee, Donald E., Horz, Friedrich, Newburn, Ray L., Zolensky, Michael, Duxbury, Thomas C., Sandford, Scott, Sekanina, Zdenek, Tsou, Peter, Hanner, Martha S., Clark, Benton C., Green, Simon F., and Kissel, Jochen
- Subjects
Stardust (Space probe) -- Equipment and supplies ,Comets -- Research -- Measurement -- Properties -- Equipment and supplies ,Science and technology ,Research ,Measurement ,Properties ,Equipment and supplies - Abstract
Images taken by the Stardust mission during its flyby of 81P/Wild 2 show the comet to be a 5-kilometer oblate body covered with remarkable topographic features, including unusual circular features that appear to be impact craters. The presence of high-angle slopes shows that the surface is cohesive and self-supporting. The comet does not appear to be a rubble pile, and its rounded shape is not directly consistent with the comet being a fragment of a larger body. The surface is active and yet it retains ancient terrain. Wild 2 appears to be in the early stages of its degradation phase as a small volatile-rich body in the inner solar system., Jupiter family comets (JFCs) such as 81 P/Wild 2 typically range from the orbit of Jupiter to inner regions of the solar system. These subliming-disintegrating bodies have inner solar system [...]
- Published
- 2004
6. EPOXI at Comet Hartley 2
- Author
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AʼHearn, Michael F., Belton, Michael J.S., Delamere, W. Alan, Feaga, Lori M., Hampton, Donald, Kissel, Jochen, Klaasen, Kenneth P., McFadden, Lucy A., Meech, Karen J., Melosh, H. Jay, Schultz, Peter H., Sunshine, Jessica M., Thomas, Peter C., Veverka, Joseph, Wellnitz, Dennis D., Yeomans, Donald K., Besse, Sebastien, Bodewits, Dennis, Bowling, Timothy J., Carcich, Brian T., Collins, Steven M., Farnham, Tony L., Groussin, Olivier, Hermalyn, Brendan, Kelley, Michael S., Li, Jian-Yang, Lindler, Don J., Lisse, Carey M., McLaughlin, Stephanie A., Merlin, Frédéric, Protopapa, Silvia, Richardson, James E., and Williams, Jade L.
- Published
- 2011
- Full Text
- View/download PDF
7. Ulysses Dust Measurements Near Jupiter
- Author
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Grün, Eberhard, Zook, Herbert A., Baguhl, Michael, Fechtig, Hugo, Hanner, Martha S., Kissel, Jochen, Lindblad, Bertil A., Linkert, Dietmar, Linkert, Gudrun, Mann, Ingrid B., Morfill, Gregor E., Polanskey, Carol, Riemann, Reiner, Schwehm, Gerhard, and Siddique, Nadeem
- Published
- 1992
8. Ulysses dust measurements near Jupiter
- Author
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Gruen, Eberhard, Zook, Herbert A, Baguhl, Michael, Fechtig, Hugo, Hanner, Martha S, Kissel, Jochen, Lindblad, Bertil A, Linkert, Dietmar, Linkert, Gudrun, and Mann, Ingrid B
- Subjects
Lunar And Planetary Exploration - Abstract
Submicrometer- to micrometer-sized particles were recorded by the Ulysses dust detector within 40 days of the Jupiter flyby. Nine impacts were recorded within 50 Jupiter radii with most of them recorded after closest approach. Three of these impacts are consistent with particles on prograde orbits around Jupiter and the rest are believed to have resulted from gravitationally focused interplanetary dust. From the ratio of the impact rate before the Jupiter flyby to the impact rate after the Jupiter flyby it is concluded that interplanetary dust particles at the distance of Jupiter move on mostly retrograde orbits. On 10 March 1992, Ulysses passed through an intense dust stream. The dust detector recorded 126 impacts within 26 hours. The stream particles were moving on highly inclined and apparently hyperbolic orbits with perihelion distances of greater than 5 astronomical units. Interplanetary dust is lost rather quickly from the solar system through collisions and other mechanisms and must be almost continuously replenished to maintain observed abundances. Dust flux measurements, therefore, give evidence of the recent rates of production from sources such as comets, asteroids, and moons, as well as the possible presence of interstellar grains.
- Published
- 1992
9. Surface of Young Jupiter Family Comet 81 P/Wild 2: Viewfrom the Stardust Spacecraft.
- Author
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Browntee, Donald E., Horz, Friedrich, Newburn, Ray L., Zolensky, Michael, Duxbury, Thomas C., Sandford, Scott, Sekanina, Zdenek, Tsou, Peter, Hanner, Martha S., Clark, Benton C., Green, Simon F., and Kissel, Jochen
- Subjects
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SPACE vehicles , *COMETS , *RUBBLE , *PHOTOGRAPHS , *SOLAR system , *ASTRONAUTICS - Abstract
Images taken by the Stardust mission during its flyby of 81P/Wild 2 show the comet to be a 5-kilometer oblate body covered with remarkable topographic features, including unusual circular features that appear to be impact craters. The presence of high-angle slopes shows that the surface is cohesive and self-supporting. The comet does not appear to be a rubble pile, and its rounded shape is not directly consistent with the comet being a fragment of a larger body. The surface is active and yet it retains ancient terrain. Wild 2 appears to be in the early stages of its degradation phase as a small volatile-rich body in the inner solar system. [ABSTRACT FROM AUTHOR]
- Published
- 2004
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