Zobrazeno 1 - 10
of 204
pro vyhledávání: '"Bannister, Michele"'
Autor:
Robinson, James E., Fitzsimmons, Alan, Young, David R., Bannister, Michele, Denneau, Larry, Erasmus, Nicolas, Lawrence, Amanda, Siverd, Robert J., Tonry, John
Sparse and serendipitous asteroid photometry obtained by wide field surveys such as the Asteroid Terrestrial-impact Last Alert System (\ATLAS) is a valuable resource for studying the properties of large numbers of small Solar System bodies. We have g
Externí odkaz:
http://arxiv.org/abs/2404.04657
The interstellar object population of the Milky Way is a product of its stars. However, what is in fact a complex structure in the Solar neighbourhood has traditionally in ISO studies been described as smoothly distributed. Using a debiased stellar p
Externí odkaz:
http://arxiv.org/abs/2402.04904
Autor:
Kareta, Theodore, Thomas, Cristina, Li, Jian-Yang, Knight, Matthew M., Moskovitz, Nicholas, Rozek, Agata, Bannister, Michele T., Ieva, Simone, Snodgrass, Colin, Pravec, Petr, Ryan, Eileen V., Ryan, William H., Fahnestock, Eugene G., Rivkin, Andrew S., Chabot, Nancy, Fitzsimmons, Alan, Osip, David, Lister, Tim, Sarid, Gal, Hirabayashi, Masatoshi, Farnham, Tony, Tancredi, Gonzalo, Michel, Patrick, Wainscoat, Richard, Weryk, Rob, Burrati, Bonnie, Pittichova, Jana, Ridden-Harper, Ryan, Tan, Nicole J., Tristram, Paul, Brown, Tyler, Bonavita, Mariangela, Burgdorf, Martin, Khalouei, Elahe, Longa, Penelope, Rabus, Markus, Sajadian, Sedighe, Jorgensen, Uffe Graae, Dominik, Martin, Kikwaya, Jean-Baptiste, Epifani, Elena Mazzotta, Dotto, Elisabetta, Deshapriya, J. D. Prasanna, Hasselmann, Pedro H., Dall'Ora, Massimo, Abe, Lyu, Guillot, Tristan, Mekarnia, Djamel, Agabi, Abdelkrim, Bendjoya, Philippe, Suarez, Olga, Triaud, Amaury, Gasparetto, Thomas, Gunther, Maximillian N., Kueppers, Michael, Merin, Bruno, Chatelain, Joseph, Gomez, Edward, Usher, Helen, Stoddard-Jones, Cai, Bartnik, Matthew, Bellaver, Michael, Chetan, Brenna, Dugan, Emma, Fallon, Tori, Fedewa, Jeremy, Gerhard, Caitlyn, Jacobson, Seth A., Painter, Shane, Peterson, David-Michael, Rodriguez, Joseph E., Smith, Cody, Sokolovsky, Kirill V., Sullivan, Hannah, Townley, Kate, Watson, Sarah, Webb, Levi, Trigo-Rodrıguez, Josep M., Llenas, Josep M., Perez-Garcıa, Ignacio, Castro-Tirado, A. J., Vincent, Jean-Baptiste, Migliorini, Alessandra, Lazzarin, Monica, La Forgia, Fiorangela, Ferrari, Fabio, Polakis, Tom, Skiff, Brian
The impact of the DART spacecraft into Dimorphos, moon of the asteroid Didymos, changed Dimorphos' orbit substantially, largely from the ejection of material. We present results from twelve Earth-based facilities involved in a world-wide campaign to
Externí odkaz:
http://arxiv.org/abs/2310.12089
Autor:
Petit, Jean-Marc, Gladman, Brett, Kavelaars, J. J., Bannister, Michele T., Alexandersen, Mike, Volk, Kathryn, Chen, Ying-Tung
Publikováno v:
ApJL 957:L4 (2023)
Using the absolute detection calibration and abundant detections of the OSSOS (Outer Solar System Origin Survey) project, we provide population measurements for the main Kuiper Belt. For absolute magnitude $H_r<8.3$, there are 30,000 non-resonant mai
Externí odkaz:
http://arxiv.org/abs/2309.01530
Autor:
Hopkins, Matthew J., Lintott, Chris, Bannister, Michele T., Mackereth, J. Ted, Forbes, John C.
Publikováno v:
AJ 166 241 (2023)
The Milky Way is thought to host a huge population of interstellar objects (ISOs), numbering approximately $10^{15}\mathrm{pc}^{-3}$ around the Sun, which are formed and shaped by a diverse set of processes ranging from planet formation to galactic d
Externí odkaz:
http://arxiv.org/abs/2308.05801
Autor:
Beaudoin, Matthew, Gladman, Brett, Huang, Yukun, Bannister, Michele, Kavelaars, J. J., Petit, Jean-Marc, Volk, Kathryn
Publikováno v:
PSJ. 4 (2022) 145
The detached transneptunian objects (TNOs) are those with semimajor axes beyond the 2:1 resonance with Neptune, which are neither resonant nor scattering. Using the detached sample from the OSSOS telescopic survey, we produce the first studies of the
Externí odkaz:
http://arxiv.org/abs/2306.12847
We calculate the upper bounds of the population of theoretically stable Centaur orbits between Uranus and Neptune. These small bodies are on low-eccentricity, low-inclination orbits in two specific bands of semi-major axis, centred at $\sim$24.6 au a
Externí odkaz:
http://arxiv.org/abs/2305.11412
Autor:
Pike, Rosemary E., Fraser, Wesley C., Schwamb, Megan E., Kavelaars, J. J., Marsset, Michael, Bannister, Michele T., Lehner, Matthew J., Wang, Shiang-Yu, Alexandersen, Mike, Chen, Ying-Tung, Gladman, Brett J., Gwyn, Stephen, Petit, Jean-Marc, Volk, Kathryn
Several different classes of trans-Neptunian objects (TNOs) have been identified based on their optical and near-infrared colors. As part of the Colours of the Outer Solar System Origins Survey (Col-OSSOS), we have obtained g-, r-, and z-band photome
Externí odkaz:
http://hdl.handle.net/10150/625819
http://arizona.openrepository.com/arizona/handle/10150/625819
http://arizona.openrepository.com/arizona/handle/10150/625819
Autor:
Shankman, Cory, Kavelaars, J. J., Bannister, Michele T., Gladman, Brett J., Lawler, Samantha M., Chen, Ying-Tung, Jakubik, Marian, Kaib, Nathan, Alexandersen, Mike, Gwyn, Stephen D. J., Petit, Jean-Marc, Volk, Kathryn
The accumulating but small set of large semimajor axis trans-Neptunian objects (TNOs) shows an apparent clustering in the orientations of their orbits. This clustering must either be representative of the intrinsic distribution of these TNOs, or else
Externí odkaz:
http://hdl.handle.net/10150/625487
http://arizona.openrepository.com/arizona/handle/10150/625487
http://arizona.openrepository.com/arizona/handle/10150/625487
Autor:
Bannister, Michele T., Shankman, Cory, Volk, Kathryn, Chen, Ying-Tung, Kaib, Nathan, Gladman, Brett J., Jakubik, Marian, Kavelaars, J. J., Fraser, Wesley C., Schwamb, Megan E., Petit, Jean-Marc, Wang, Shiang-Yu, Gwyn, Stephen D. J., Alexandersen, Mike, Pike, Rosemary E.
We report the discovery of the minor planet 2013 SY99 on an exceptionally distant, highly eccentric orbit. With a perihelion of 50.0. au, 2013 SY99' s orbit has a semimajor axis of 730 +/- 40. au, the largest known for a high-perihelion trans-Neptuni
Externí odkaz:
http://hdl.handle.net/10150/624444
http://arizona.openrepository.com/arizona/handle/10150/624444
http://arizona.openrepository.com/arizona/handle/10150/624444