Zobrazeno 1 - 10
of 389
pro vyhledávání: '"Young, Edward D"'
Autor:
Spitzer, Fridolin, Kleine, Thorsten, Burkhardt, Christoph, Hopp, Timo, Yokoyama, Tetsuya, Abe, Yoshinari, Aléon, Jérôme, Alexander, Conel M. O'D., Amari, Sachiko, Amelin, Yuri, Bajo, Ken-ichi, Bizzarro, Martin, Bouvier, Audrey, Carlson, Richard W., Chaussidon, Marc, Choi, Byeon-Gak, Dauphas, Nicolas, Davis, Andrew M., Di Rocco, Tommaso, Fujiya, Wataru, Fukai, Ryota, Gautam, Ikshu, Haba, Makiko K., Hibiya, Yuki, Hidaka, Hiroshi, Homma, Hisashi, Hoppe, Peter, Huss, Gary R., Ichida, Kiyohiro, Iizuka, Tsuyoshi, Ireland, Trevor R., Ishikawa, Akira, Itoh, Shoichi, Kawasaki, Noriyuki, Kita, Noriko T., Kitajima, Kouki, Komatani, Shintaro, Krot, Alexander N., Liu, Ming-Chang, Masuda, Yuki, Morita, Mayu, Moynier, Fréderic, Motomura, Kazuko, Nakai, Izumi, Nagashima, Kazuhide, Nguyen, Ann, Nittler, Larry, Onose, Morihiko, Pack, Andreas, Park, Changkun, Piani, Laurette, Qin, Liping, Russell, Sara S., Sakamoto, Naoya, Schönbächler, Maria, Tafla, Lauren, Tang, Haolan, Terada, Kentaro, Terada, Yasuko, Usui, Tomohiro, Wada, Sohei, Wadhwa, Meenakshi, Walker, Richard J., Yamashita, Katsuyuki, Yin, Qing-Zhu, Yoneda, Shigekazu, Young, Edward D., Yui, Hiroharu, Zhang, Ai-Cheng, Nakamura, Tomoki, Naraoka, Hiroshi, Noguchi, Takaaki, Okazaki, Ryuji, Sakamoto, Kanako, Yabuta, Hikaru, Abe, Masanao, Miyazaki, Akiko, Nakato, Aiko, Nishimura, Masahiro, Okada, Tatsuaki, Yada, Toru, Yogata, Kasumi, Nakazawa, Satoru, Saiki, Takanao, Tanaka, Satoshi, Terui, Fuyuto, Tsuda, Yuichi, Watanabe, Sei-ichiro, Yoshikawa, Makoto, Tachibana, Shogo, Yurimoto, Hisayoshi
Publikováno v:
Science Advances 10, 39, eadp2426 (2024)
The isotopic compositions of samples returned from Cb-type asteroid Ryugu and Ivuna-type (CI) chondrites are distinct from other carbonaceous chondrites, which has led to the suggestion that Ryugu and CI chondrites formed in a different region of the
Externí odkaz:
http://arxiv.org/abs/2410.04192
Autor:
Rogers, James G., Dorn, Caroline, Raj, Vivasvaan Aditya, Schlichting, Hilke E., Young, Edward D.
Super-Earths are highly irradiated, small planets with bulk densities approximately consistent with Earth. We construct combined interior-atmosphere models of super-Earths that trace the partitioning of water throughout a planet, including an iron-ri
Externí odkaz:
http://arxiv.org/abs/2409.17394
We investigate the consequences of non-ideal chemical interaction between silicate and overlying hydrogen-rich envelopes for rocky planets using basic tenets of phase equilibria. Based on our current understanding of the temperature and pressure cond
Externí odkaz:
http://arxiv.org/abs/2408.11321
Autor:
Hinkel, Natalie R., Young, Edward D.
The relationship between stars and planets provides important information for understanding the interior composition, mineralogy, and overall classification of small planets (R $\lesssim$ 3.5R$_{\oplus}$). Since stars and planets are formed at the sa
Externí odkaz:
http://arxiv.org/abs/2405.05324
Autor:
Benneke, Björn, Roy, Pierre-Alexis, Coulombe, Louis-Philippe, Radica, Michael, Piaulet, Caroline, Ahrer, Eva-Maria, Pierrehumbert, Raymond, Krissansen-Totton, Joshua, Schlichting, Hilke E., Hu, Renyu, Yang, Jeehyun, Christie, Duncan, Thorngren, Daniel, Young, Edward D., Pelletier, Stefan, Knutson, Heather A., Miguel, Yamila, Evans-Soma, Thomas M., Dorn, Caroline, Gagnebin, Anna, Fortney, Jonathan J., Komacek, Thaddeus, MacDonald, Ryan, Raul, Eshan, Cloutier, Ryan, Acuna, Lorena, Lafrenière, David, Cadieux, Charles, Doyon, René, Welbanks, Luis, Allart, Romain
Even though sub-Neptunes likely represent the most common outcome of planet formation, their natures remain poorly understood. In particular, planets near 1.5-2.5$\,R_\oplus$ often have bulk densities that can be explained equally well with widely di
Externí odkaz:
http://arxiv.org/abs/2403.03325
Small, close-in exoplanets are divided into two sub-populations: super-Earths and sub-Neptunes. Most super-Earths are thought to have lost their primordially accreted hydrogen-dominated atmospheres via thermally driven winds. We consider the global c
Externí odkaz:
http://arxiv.org/abs/2402.14072
Autor:
Tissot, François L. H., Ibañez-Mejia, Mauricio, Rabb, Savelas A., Kraft, Rebecca A., Vocke, Robert D., Fehr, Manuela A., Schönbächler, Maria, Tang, Haolan, Young, Edward D.
Publikováno v:
Journal of Analytical Atomic Spectrometry, 38(10), pp.2087-2104 (2023)
As the field of Zr stable isotopes is rapidly expanding from the study of mass-independent to that of mass-dependent isotope effects, a variety of Zr standards have appeared in the literature. While several of these standards have been proposed as th
Externí odkaz:
http://arxiv.org/abs/2404.14413
A persistent question in exoplanet demographics is whether exoplanetary systems form from similar compositional building blocks to our own. Polluted white dwarf stars offer a unique way to address this question as they provide measurements of the bul
Externí odkaz:
http://arxiv.org/abs/2306.03743
Publikováno v:
Nature, v. 616 (7956), 306-311 (2023)
Earth's water, intrinsic oxidation state, and metal core density are fundamental chemical features of our planet. Studies of exoplanets provide a useful context for elucidating the source of these chemical traits. Planet formation and evolution model
Externí odkaz:
http://arxiv.org/abs/2304.07845
Sub-Neptune exoplanets are commonly hypothesized to consist of a silicate-rich magma ocean topped by a hydrogen-rich atmosphere. Previous work studying the outgassing of silicate material has demonstrated that such atmosphere-interior interactions ca
Externí odkaz:
http://arxiv.org/abs/2303.09653