Results 81 to 90 of about 1,643,192 (137)

86th Annual Meeting of the Meteoritical Society (2024)

Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley   +1 more source

Pluto near the edge of chaos. [PDF]

Proc Natl Acad Sci U S A, 2022
Malhotra R, Ito T.
europepmc   +1 more source

Machine Learning Classification of Kuiper Belt Populations. [PDF]

Mon Not R Astron Soc, 2020
Smullen RA, Volk K.
europepmc   +1 more source

Organic Components of Small Bodies in the Outer Solar System: Some Results of the New Horizons Mission. [PDF]

Life (Basel), 2020
Cruikshank DP, Pendleton YJ, Grundy WM.
europepmc   +1 more source

Orbital stability analysis and photometric characterization of the second Earth Trojan asteroid 2020 XL₅. [PDF]

Nat Commun, 2022
Santana-Ros T, Micheli M, Faggioli L, Cennamo R, Devogèle M, Alvarez-Candal A, Oszkiewicz D, Ramírez O, Liu PY, Benavidez PG, Campo Bagatin A, Christensen EJ, Wainscoat RJ, Weryk R, Fraga L, Briceño C, Conversi L.   +16 more
europepmc   +1 more source

A collisional family of icy objects in the Kuiper belt [PDF]

, 2007
The small bodies in the Solar System are thought to have been highly affected by collisions and erosion. In the asteroid belt, direct evidence of the effects of large collisions can be seen in the existence of separate families of asteroids—a family ...
Ragozzine, Darin, Schaller, Emily L., Barkume, Kristina, Brown, Michael E.   +3 more
core  

Spectrophotometric Observations of Edgeworth-Kuiper Belt Objects

, 1999
The Edgeworth-Kuiper Belt (EKB) objects are fossil remnants of the formation of the Solar System and they represent an important reservoir of primordial, thermally unprocessed material. The study of these objects has rapidly evolved in the last few years.
BARUCCI M. A., THOLEN D., LAZZARIN, MONICA, FULCHIGNONI M., DORESSOUNDIRAM A.   +4 more
core   +1 more source

Size and albedo of Kuiper belt object 55636 from a stellar occultation

, 2010
The Kuiper belt is a collection of small bodies (Kuiper belt objects, KBOs) that lie beyond the orbit of Neptune and which are believed to have formed contemporaneously with the planets.
Lockhart, M, Kakkala, M., Levine, S, Zangari, A.M., Grigsby, B., M. J. Person, DuPré, K., Ryan, W. H., E. R. Adams, J. Wolf, G. Jacobson, A. A. S. Gulbis, Rapoport, Sharon, E. W. Dunham, Zangari, A. M., Mattingly, A., Pasachoff, J.M., Zuluaga, C.A., Zuluaga, C. A., Lockhart, M., Sheppard, S.S., Zangari, A, A. S. Bosh, Berger, B., Ragozzine, D., Person, M.J., E. V. Ryan, Ryan, W.H., Michel, R., Bosh, A.S., L. Bright, Ryan, E.V., Briggs, J. W., Gilmore, A., W. Rosing, B. A. Babcock, Babcock, B.A., Bosh, A S, Wolf, J., Elliot, J, B. Volz, J. M. Pasachoff, A. Mattingly, Elliot, J. L., Adams, E. R., A. M. Zangari, Jacobson, G., S. S. Sheppard, Gulbis, A. A. S., M. Kakkala, Brucker, M., N. Secrest, Secrest, N., K. DuPré, Tilleman, T., Levine, S.E., Montano, H.G., Briggs, J.W., A. W. Meyer, R. Michel, Adams, E.R., J. Brimacombe, Valleli, P., Rapoport, S., Person, M, S. E. Levine, P. Valleli, Brothers, T.C., Souza, S. P., C. A. Zuluaga, Montano, H. G., Brothers, T. C., Bright, L., Bosh, A. S., Brothers, T C, Dunham, E.W., Rosing, W., A. Gilmore, J. W. Briggs, Meyer, A. W., Dunham, E. W., Zambrano-Marin, L., B. Grigsby, T. Tilleman, Pasachoff, J. M., Hart, R., R. Hart, M. Lockhart, B. Berger, Morzinski, K., Volz, B., Meyer, A.W., Person, M. J., K. Morzinski, S. P. Souza, Babcock, B. A., Souza, S.P., H. G. Montano, Sheppard, S. S., S. Rapoport, L. Zambrano-Marin, Levine, S. E., T. C. Brothers, M. Brucker, Ryan, E. V., W. H. Ryan, Elliot, J.L., Brimacombe, J., J. L. Elliot, Gulbis, A.A.S., D. Ragozzine   +110 more
core   +1 more source

Long-Term Dynamics And The Orbital Inclinations Of The Classical

, 2007
We numerically integrated the orbits of 1458 particles in the region of the classical Kuiper belt (41 AU a 47 AU) to explore the role of dynamical instabilities in sculpting the inclination distribution of the classical Kuiper belt objects (KBOs).
Matthew Holman, Kuiper Belt Objects, Michael E. Brown   +2 more
core  

Cosmic Ray Mantle Visibility on Kuiper Belt Objects

, 2006
Optically red objects constitute the dynamically cold, old component of the Classical Kuiper Belt (40 - 47 AU) with heliocentric orbits of low eccentricity and inclination.
Sturner, S. J., Hill, Matt E., Cooper, John F., Richardson, J. D.   +3 more
core