Results 11 to 20 of about 304,444 (325)
The fragility of planetary systems [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 We specify the range to which perturbations penetrate a planetesimal system.
Such perturbations can originate from massive planets or from encounters with
other stars.Jilkova, Lucie, Zwart, Simon Portegiescore +7 more sourcesDusty Planetary Systems [PDF]
, 2012 Extensive photometric stellar surveys show that many main sequence stars show
emission at infrared and longer wavelengths that is in excess of the stellar
photosphere; this emission is thought to arise from circumstellar dust.A Moro-Martín, A Moro-Martín, A Moro-Martín, A Moro-Martín, A Moro-Martín, A Moro-Martín, A Moro-Martín, A-M Lagrange, AC Quillen, AV Krivov, AV Krivov, BAS Gustafson, C Dominik, C Eiroa, C Lovis, C Vitense, CA Beichman, CA Beichman, CC Stark, CD Murray, CF Chyba, CH Chen, CM Lisse, CR Chapman, D Brownlee, D Jewitt, D Jewitt, D Mouillet, DA Fischer, DA Gurnett, DE Backman, DE Trilling, E Chiang, E Grün, EK Jessberger, FY Morales, G Bryden, G Bryden, G Decin, G Marcy, G Schneider, GH Rieke, GM Bernstein, HA Zook, HH Aumann, HJ Habing, J Wisdom, J-C Liou, JA Burns, JC Weingartner, JE Krist, JH Debes, JM Carpenter, JR Houck, JS Dohnanyi, JS Greaves, JS Greaves, JS Greaves, JS Greaves, JS Mathis, KA Farley, KD McKeegan, KR Stapelfeldt, KY L Su, KY L Su, LA Hillenbrand, M Booth, M Clampin, M Jura, M Jura, M Landgraf, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, MC Wyatt, ME Zolensky, MF A’Hearn, MR Meyer, MV Sykes, N Siegler, P Kalas, P Kalas, P Kalas, P Plavchan, P Thébault, PC Frisch, R Gomes, R Malhotra, RG Strom, S Müller, S Yamamoto, SA Sandford, SA Stern, SF Dermott, SJ Kenyon, SN Raymond, T Löhne, TN Gautier III, W Benz, WF Bottke, WS Holland, WS Holland, WT Reach, WT Reach, ZM Leinhardt, Á Kóspál +106 morecore +3 more sourcesThe (In)Stability of Planetary Systems [PDF]
The Astrophysical Journal, 2004 We present results of numerical simulations which examine the dynamical
stability of known planetary systems, a star with two or more planets. First we
vary the initial conditions of each system based on observational data.Chambers J. E., Duncan M. J., Gonzalez G., Laskar J., Rory Barnes, Santos N. C., Thomas Quinn +6 morecore +4 more sourcesForming Different Planetary Systems [PDF]
Research in Astronomy and Astrophysics, 2012 With the increasing number of detected exoplanet samples, the statistical
properties of planetary systems have become much clearer. In this review, we
summarize the major statistics that have been revealed mainly by radial
velocity and transiting ...Armitage, Batalha, Batygin, Binney, Borucki, Burkert, Butler, Butler, Chatterjee, Cieza, Cuzzi, Dawson, Duquennoy, Eggenberger, Endl, Fabrycky, Fabrycky, Fischer, Ford, Ford, Fortney, Fregeau, Gaudi, Gilliland, Gonzalez, Gould, Guedes, Haghighipour, Haghighipour, Haisch, Hatzes, Heppenheimer, Hernández, Holman, Howard, Hui Zhang, Hui-Gen Liu, Ida, Ida, Ida, Ida, Ikoma, Jang-Condell, Ji-Lin Zhou, Ji-Wei Xie, Johnson, Johnson, Jurić, Kaib, Kennedy, Kley, Kley, Kokubo, Kratter, Larwood, Laughlin, Lee, Lee, Levison, Lithwick, Lithwick, Liu, Marcy, Marti, Marzari, Marzari, Matsumura, Matsuyama, Mayer, Mayor, Mayor, Meschiari, Mochejska, Murray, Nagasawa, Nagasawa, Nagasawa, Naoz, Ormel, Pascucci, Perets, Perets, Pfahl, Pätzold, Qian, Queloz, Quinn, Quintana, Quintana, Rafikov, Rafikov, Raghavan, Raghavan, Rosvick, Saleh, Sato, Schlaufman, Socrates, Sozzetti, Spurzem, Stewart, Takeda, Tanaka, Terquem, Tremaine, Wang, Wang, Weidenschilling, Weldrake, Weldrake, Winn, Wittenmyer, Wittenmyer, Wittenmyer, Wright, Wright, Wright, Wu, Wu, Wu, Xie, Xie, Xie, Xie, Yasui, Yi-Sui Sun, Youdin, Zhang, Zhang, Zhao, Zhou, Zhou, Zhou, Zucker, Zucker +134 morecore +3 more sourcesThe birth environment of planetary systems. [PDF]
R Soc Open Sci, 2020 Star and planet formation are inextricably linked. In the earliest phases of the collapse of a protostar, a disc forms around the young star and such discs are observed for the first several million years of a star’s life. It is within these circumstellar, or protoplanetary, discs that the first stages of planet formation occur.Parker RJ.europepmc +8 more sourcesThe formation of planetary systems with SPICA [PDF]
Publications of the Astronomical Society of Australia, 2021 Abstract In this era of spatially resolved observations of planet-forming disks with Atacama Large Millimeter Array (ALMA) and large ground-based telescopes such as the Very Large Telescope (VLT), Keck, and Subaru, we still lack statistically relevant information on the quantity and composition of the material that is building the planets, such as ...Kamp, I., Honda, M., Nomura, H., Audard, M., Fedele, D., Waters, L. B. F. M., Aikawa, Y., Banzatti, A., Bowey, J. E., Bradford, M., Dominik, C., Furuya, K., Habart, E., Ishihara, D., Johnstone, D., Kennedy, G., Kim, M., Kral, Q., Lai, S. P., Larsson, B., McClure, M., Miotello, A., Momose, M., Nakagawa, T., Naylor, D., Nisini, B., Notsu, S., Onaka, T., Pantin, E., Podio, L., Marichalar, P. Riviere, Rocha, W. R. M., Roelfsema, P., Santos, F., Shimonishi, T., Tang, Y. W., Takami, M., Tazaki, R., Wolf, S., Wyatt, M., Ysard, N. +40 moreopenaire +9 more sourcesPlanetary Systems Biology [PDF]
Molecular Cell, 2005 Combining paleogenetics, protein engineering, synthetic biology, and metabolic modeling, a planetary biology perspective is brought to bear on adaptive evolutionary events in ancient bacteria.Department of Chemistry, University of Florida, Gainesville, FL 32611 USA ( host institution ), Benner, Steven A., Ricardo, Alonso +2 moreopenaire +4 more sourcesA Quantitative Comparison of Exoplanet Catalogs
Geosciences, 2018 In this study, we investigated the differences between four commonly-used exoplanet catalogs (exoplanet.eu; exoplanetarchive.ipac.caltech.edu; openexoplanetcatalogue.com; exoplanets.org) using a Kolmogorov–Smirnov (KS) test.Dolev Bashi, Ravit Helled, Shay Zuckerdoaj +1 more sourcePaleo‐Permeability Structure of the Crustal Section of the Samail Ophiolite Based on Automated Detection of Veins in X‐Ray CT Core Images From the Oman Drilling Project
Geochemistry, Geophysics, Geosystems, 2023 To assess the paleo‐permeability structure of oceanic crust, we used 3‐D X‐ray Computed Tomography (XCT) images to quantify the distribution and geometry of mineral veins in core samples from Oman Drilling Project Holes GT1A, GT2A, and GT3A, which ...Y. Akamatsu, I. Katayama, K. Okazaki, K. Michibayashi +3 moredoaj +1 more source