Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1029/2019GL085746 |
Tides on Other Earths: Implications for Exoplanet and Palaeo-Tidal Simulations | |
Blackledge, B. W.1; Green, J. A. M.1; Barnes, R.2; Way, M. J.3,4,5 | |
2020-05-30 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS
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ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2020 |
卷号 | 47期号:12 |
文章类型 | Article |
语种 | 英语 |
国家 | Wales; USA; Sweden |
英文摘要 | A key controller of a planet's rotational evolution, and hence habitability, is tidal dissipation, which on Earth is dominated by the ocean tides. Because exoplanet or deep-time Earth topographies are unknown, a statistical ensemble is used to constrain possible tidal dissipation rates on an Earth-like planet. A dedicated tidal model is used together with 120 random continental configurations to simulate Earth's semidiurnal lunar tide. The results show a possible ocean tidal dissipation range spanning 3 orders of magnitude, between 2.3 GW to 1.9 TW (1 TW=10(12) W). When model resolution is considered, this compares well with theoretical limits derived for the energetics of Earth's present-day deep ocean. Consequently, continents exert a fundamental control on tidal dissipation rates and we suggest that plate tectonics on a planet will induce a time-varying dissipation analogous to Earth's. This will alter rotational periods over millions of years and further complicate the role of tides for planetary evolution. Plain Language Summary The daylength of a planet is key for habitability because it regulates the rate with which solar radiation is received and redistributed at the surface. A main controller of a planet's daylength is the ocean tide, because the dissipation of tidal energy works as a brake on the planet's spin, increasing the daylength. Tides are sensitive to the continental arrangement on a planet, but there are no details of the surface of any exoplanet and only limited information of what Earth looked like in the distant past. The change in Earth's daylength forces the Moon to recede into a higher orbit, but the present-day recession rate is very high and does not fit our age models of the moon, implying that the tides must have been much weaker in the distant past. Here, we use a series of tidal predictions for random continental configurations of Earth to provide a range of tidal dissipation rates and thus an estimate of how the tides in the deep past may have evolved as Earth's continents grew more and more complex. This research also provides a range of dissipation rates that can be used for simulations of the rotational and orbital evolution of exoplanets. |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000551464800014 |
WOS关键词 | EVOLUTION ; DISSIPATION ; ENERGY |
WOS类目 | Geosciences, Multidisciplinary |
WOS研究方向 | Geology |
URL | 查看原文 |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/271604 |
专题 | 气候变化 |
作者单位 | 1.Bangor Univ, Sch Ocean Sci, Menai Bridge, Gwynedd, Wales; 2.Univ Washington, Dept Astron, Seattle, WA 98195 USA; 3.NASA, Goddard Inst Space Studies, New York, NY 10025 USA; 4.Goddard Space Flight Ctr, Sellers Exoplanet Environm, Greenbelt, MD USA; 5.Uppsala Univ, Dept Phys & Astron, Theoret Astrophys, Uppsala, Sweden |
推荐引用方式 GB/T 7714 | Blackledge, B. W.,Green, J. A. M.,Barnes, R.,et al. Tides on Other Earths: Implications for Exoplanet and Palaeo-Tidal Simulations[J]. GEOPHYSICAL RESEARCH LETTERS,2020,47(12). |
APA | Blackledge, B. W.,Green, J. A. M.,Barnes, R.,&Way, M. J..(2020).Tides on Other Earths: Implications for Exoplanet and Palaeo-Tidal Simulations.GEOPHYSICAL RESEARCH LETTERS,47(12). |
MLA | Blackledge, B. W.,et al."Tides on Other Earths: Implications for Exoplanet and Palaeo-Tidal Simulations".GEOPHYSICAL RESEARCH LETTERS 47.12(2020). |
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