Pluto’s interaction with its space environment: Solar wind, energetic particles, and dust
Author:
Bagenal F.1, Horányi M.1, McComas D. J.23, McNutt R. L.4, Elliott H. A.2, Hill M. E.4, Brown L. E.4, Delamere P. A.5, Kollmann P.4, Krimigis S. M.46, Kusterer M.4, Lisse C. M.4, Mitchell D. G.4, Piquette M.1, Poppe A. R.7, Strobel D. F.8, Szalay J. R.19, Valek P.2, Vandegriff J.4, Weidner S.2, Zirnstein E. J.2, Stern S. A.9, Ennico K.10, Olkin C. B.9, Weaver H. A.4, Young L. A.9, Gladstone G. R., Grundy W. M., McKinnon W. B., Moore J. M., Spencer J. R., Andert T., Andrews J., Banks M., Bauer B., Bauman J., Barnouin O. S., Bedini P., Beisser K., Beyer R. A., Bhaskaran S., Binzel R. P., Birath E., Bird M., Bogan D. J., Bowman A., Bray V. J., Brozovic M., Bryan C., Buckley M. R., Buie M. W., Buratti B. J., Bushman S. S., Calloway A., Carcich B., Cheng A. F., Conard S., Conrad C. A., Cook J. C., Cruikshank D. P., Custodio O. S., Dalle Ore C. M., Deboy C., Dischner Z. J. B., Dumont P., Earle A. M., Ercol J., Ernst C. M., Finley T., Flanigan S. H., Fountain G., Freeze M. J., Greathouse T., Green J. L., Guo Y., Hahn M., Hamilton D. P., Hamilton S. A., Hanley J., Harch A., Hart H. M., Hersman C. B., Hill A., Hinson D. P., Holdridge M. E., Howard A. D., Howett C. J. A., Jackman C., Jacobson R. A., Jennings D. E., Kammer J. A., Kang H. K., Kaufmann D. E., Kusnierkiewicz D., Lauer T. R., Lee J. E., Lindstrom K. L., Linscott I. R., Lunsford A. W., Mallder V. A., Martin N., Mehoke D., Mehoke T., Melin E. D., Mutchler M., Nelson D., Nimmo F., Nunez J. I., Ocampo A., Owen W. M., Paetzold M., Page B., Parker A. H., Parker J. W., Pelletier F., Peterson J., Pinkine N., Porter S. B., Protopapa S., Redfern J., Reitsema H. J., Reuter D. C., Roberts J. H., Robbins S. J., Rogers G., Rose D., Runyon K., Retherford K. D., Ryschkewitsch M. G., Schenk P., Schindhelm E., Sepan B., Showalter M. R., Singer K. N., Soluri M., Stanbridge D., Steffl A. J., Stryk T., Summers M. E., Tapley M., Taylor A., Taylor H., Throop H. B., Tsang C. C. C., Tyler G. L., Umurhan O. M., Verbiscer A. J., Versteeg M. H., Vincent M., Webbert R., Weigle G. E., White O. L., Whittenburg K., Williams B. G., Williams K., Williams S., Woods W. W., Zangari A. M.,
Affiliation:
1. Laboratory of Atmospheric and Space Physics, University of Colorado, Boulder, CO 80600, USA. 2. Southwest Research Institute, San Antonio, TX 78228, USA. 3. University of Texas at San Antonio, San Antonio, TX 78249, USA. 4. Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA. 5. University of Alaska, Fairbanks, AK 99775, USA. 6. Academy of Athens, 28 Panapistimiou, 10679 Athens, Greece. 7. Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA. 8. Johns Hopkins University, Baltimore, MD 21218, USA. 9. Southwest Research Institute, Boulder, CO 80302, USA. 10. NASA Ames Research Center, Moffett Field, CA 94035, USA.
Abstract
New Horizons unveils the Pluto system
In July 2015, the New Horizons spacecraft flew through the Pluto system at high speed, humanity's first close look at this enigmatic system on the outskirts of our solar system. In a series of papers, the New Horizons team present their analysis of the encounter data downloaded so far: Moore
et al.
present the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes. Grundy
et al.
analyzed the colors and chemical compositions of their surfaces, with ices of H
2
O, CH
4
, CO, N
2
, and NH
3
and a reddish material which may be tholins. Gladstone
et al.
investigated the atmosphere of Pluto, which is colder and more compact than expected and hosts numerous extensive layers of haze. Weaver
et al.
examined the small moons Styx, Nix, Kerberos, and Hydra, which are irregularly shaped, fast-rotating, and have bright surfaces. Bagenal
et al.
report how Pluto modifies its space environment, including interactions with the solar wind and a lack of dust in the system. Together, these findings massively increase our understanding of the bodies in the outer solar system. They will underpin the analysis of New Horizons data, which will continue for years to come.
Science
, this issue pp.
1284
,
10.1126/science.aad9189
,
10.1126/science.aad8866
,
10.1126/science.aae0030
, &
10.1126/science.aad9045
Publisher
American Association for the Advancement of Science (AAAS)
Subject
Multidisciplinary
Cited by
60 articles.
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