Zobrazeno 1 - 10
of 6 222
pro vyhledávání: '"Stern, S"'
Autor:
Fraser, Wesley C., Porter, Simon B., Peltier, Lowell, Kavelaars, JJ, Verbiscer, Anne J., Buie, Marc W., Stern, S. Alan, Spencer, John R., Benecchi, Susan D., Terai, Tsuyoshi, Ito, Takashi, Yoshida, Fumi, Gerdes, David W., Napier, Kevin J., Lin, Hsing Wen, Gwyn, Stephen D. J., Smotherman, Hayden, Fabbro, Sebastien, Singer, Kelsi N., Alexander, Amanda M., Arimatsu, Ko, Banks, Maria E., Bray, Veronica J., El-Maarry, Mohamed Ramy, Ferrell, Chelsea L., Fuse, Tetsuharu, Glass, Florian, Holt, Timothy R., Hong, Peng, Ishimaru, Ryo, Johnson, Perianne E., Lauer, Tod R., Leiva, Rodrigo, Lykawka, Patryk S., Marschall, Raphael, Núñez, Jorge I., Postman, Marc, Quirico, Eric, Rhoden, Alyssa R., Simpson, Anna M., Schenk, Paul, Skrutskie, Michael F., Steffl, Andrew J., Throop, Henry
We report the detection of 239 trans-Neptunian Objects discovered through the on-going New Horizons survey for distant minor bodies being performed with the Hyper Suprime-Cam mosaic imager on the Subaru Telescope. These objects were discovered in ima
Externí odkaz:
http://arxiv.org/abs/2407.21142
Autor:
Postman, Marc, Lauer, Tod R., Parker, Joel W., Spencer, John R., Weaver, Harold A., Shull, J. Michael, Stern, S. Alan, Brandt, Pontus, Conard, Steven J., Gladstone, G. Randall, Lisse, Carey M., Porter, Simon D., Singer, Kelsi N., Verbiscer, Anne J.
We obtained New Horizons LORRI images to measure the cosmic optical background (COB) intensity integrated over $0.4\lesssim\lambda\lesssim0.9{~\rm\mu m}.$ The survey comprises 16 high Galactic-latitude fields selected to minimize scattered diffuse Ga
Externí odkaz:
http://arxiv.org/abs/2407.06273
Autor:
Buie, Marc W., Spencer, John R., Porter, Simon B., Benecchi, Susan D., Parker, Alex H., Stern, S. Alan, Belton, Michael, Binzel, Richard P., Borncamp, David, DeMeo, Francesca, Fabbro, S., Fuentes, Cesar, Furusawa, Hisanori, Fuse, Tetsuharu, Gay, Pamela L., Gwyn, Stephen, Holman, Matthew J., Karoji, H., Kavelaars, J. J., Kinoshita, Daisuke, Miyazaki, Satoshi, Mountain, Matt, Noll, Keith S., Osip, David J., Petit, Jean-Marc, Reid, Neill I., Sheppard, Scott S., Showalter, Mark, Steffl, Andrew J., Sterner, Ray E., Tajitsu, Akito, Tholen, David J., Trilling, David E., Weaver, Harold A., Verbiscer, Anne J., Wasserman, Lawrence H., Yamashita, Takuji, Yanagisawa, Toshifumi, Yoshida, Fumi, Zangari, Amanda M.
Following the Pluto fly-by of the New Horizons spacecraft, the mission provided a unique opportunity to explore the Kuiper Belt in-situ. The possibility existed to fly-by a Kuiper Belt object (KBO) as well as to observe additional objects at distance
Externí odkaz:
http://arxiv.org/abs/2403.04927
Autor:
Doner, Alex, Horanyi, Mihaly, Bagenal, Fran, Brandt, Pontus, Grundy, Will, Lisse, Carey, Parker, Joel, Poppe, Andrew R., Singer, Kelsi N., Stern, S. Alan, Verbiscer, Anne
The NASA New Horizons Venetia Burney Student Dust Counter (SDC) measures dust particle impacts along the spacecraft's flight path for grains with mass $\ge$ $10^{-12}$ g, mapping out their spatial density distribution. We present the latest SDC dust
Externí odkaz:
http://arxiv.org/abs/2401.01230
Autor:
Stern, S. A., White, O. L., Grundy, Wm., Keeney, B. A., Hofgartner, J. D., Nesvorny, D., McKinnon, W. B., Richardson, D. C., Marohnic, J. C., Verbiscer, A. J., Benecchi, S. D., Schenk, P. M., Moore, J. M.
We report on a study of the mounds that dominate the appearance of Kuiper Belt Object (KBO) (486958) Arrokoth's larger lobe, named Wenu. We compare the geological context of these mounds, measure and intercompare their shapes, sizes/orientations, ref
Externí odkaz:
http://arxiv.org/abs/2308.16834
Autor:
Robbins, Stuart J., Runyon, Kirby, Singer, Kelsi N., Bray, Veronica J., Beyer, Ross A., Schenk, Paul, McKinnon, William B., Grundy, William M., Nimmo, Francis, Moore, Jeffrey M., Spencer, John R., White, Oliver L., Binzel, Richard P., Buie, Marc W., Buratti, Bonnie J., Cheng, Andrew F., Linscott, Ivan R., Reitsema, Harold J., Reuter, Dennis C., Showalter, Mark R., Tyler, G. Len, Young, Leslie A., Olkin, Catherine B., Ennico, Kimberly S., Weaver, Harold A., Stern, S. Alan
On the moon and other airless bodies, ballistically emplaced ejecta transitions from a thinning, continuous inner deposit to become discontinuous beyond approximately one crater radius from the crater rim and can further break into discrete rays and
Externí odkaz:
http://hdl.handle.net/10150/627125
http://arizona.openrepository.com/arizona/handle/10150/627125
http://arizona.openrepository.com/arizona/handle/10150/627125
Autor:
Singer, Kelsi N., White, Oliver L., Schmitt, Bernard, Rader, Erika L., Protopapa, Silvia, Grundy, William M., Cruikshank, Dale P., Bertrand, Tanguy, Schenk, Paul M., McKinnon, William B., Stern, S. Alan, Dhingra, Rajani D., Runyon, Kirby D., Beyer, Ross A., Bray, Veronica J., Ore, Cristina Dalle, Spencer, John R., Moore, Jeffrey M., Nimmo, Francis, Keane, James T., Young, Leslie A., Olkin, Catherine B., Lauer, Tod R., Weaver, Harold A., Ennico-Smith, Kimberly
Publikováno v:
Nature Communications 13, 1542 (2022)
The New Horizons spacecraft returned images and compositional data showing that terrains on Pluto span a variety of ages, ranging from relatively ancient, heavily cratered areas to very young surfaces with few-to-no impact craters. One of the regions
Externí odkaz:
http://arxiv.org/abs/2207.06557
Autor:
Lisse, C. M., Gladstone, G. R., 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., Parker, J. M., Binzel, R. P., Earle, A. M., Horanyi, M., El-Maarry, M., 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.
We present new, ice species-specific New Horizons/Alice upper gas coma production limits from the 01 Jan 2019 MU69/Arrokoth flyby of Gladstone et al. (2021) and use them to make predictions about the rarity of majority hypervolatile (CO, N$_2$, CH$_4
Externí odkaz:
http://arxiv.org/abs/2203.08888
Autor:
Umurhan, O. M., Grundy, W. M., Bird, M. K., Beyer, R., Keane, J. T., Linscott, I. R., Birch, S., Bierson, C., Young, L. A., Stern, S. A., Lisse, C. M., Howett, C. J. A., Protopapa, S., Spencer, J. R., Binzel, R. P., Mckinnon, W. B., Lauer, T. R., Weaver, H. A., Olkin, C. B., Singer, K. N., Verbiscer, A. J., Parker, A. H.
A near surface thermal model for Arrokoth is developed based on the recently released $10^5$ facet model of the body. This thermal solution takes into account Arrokoth's surface re-radiation back onto itself. The solution method exploits Arrokoth's p
Externí odkaz:
http://arxiv.org/abs/2202.10485