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DOI | 10.1126/science.aar7268 |
Radar evidence of subglacial liquid water on Mars | |
Orosei R.; Lauro S.E.; Pettinelli E.; Cicchetti A.; Coradini M.; Cosciotti B.; Di Paolo F.; Flamini E.; Mattei E.; Pajola M.; Soldovieri F.; Cartacci M.; Cassenti F.; Frigeri A.; Giuppi S.; Martufi R.; Masdea A.; Mitri G.; Nenna C.; Noschese R.; Restano M.; Seu R. | |
发表日期 | 2018 |
ISSN | 0036-8075 |
起始页码 | 490 |
结束页码 | 493 |
卷号 | 361期号:6401 |
英文摘要 | The presence of liquid water at the base of the martian polar caps has long been suspected but not observed. We surveyed the Planum Australe region using the MARSIS (Mars Advanced Radar for Subsurface and Ionosphere Sounding) instrument, a low-frequency radar on the Mars Express spacecraft. Radar profiles collected between May 2012 and December 2015 contain evidence of liquid water trapped below the ice of the South Polar Layered Deposits. Anomalously bright subsurface reflections are evident within a well-defined, 20-kilometer-wide zone centered at 193°E, 81°S, which is surrounded by much less reflective areas. Quantitative analysis of the radar signals shows that this bright feature has high relative dielectric permittivity (>15), matching that of water-bearing materials. We interpret this feature as a stable body of liquid water on Mars. © 2017 The Authors. |
英文关键词 | calcium; carbon dioxide; ice; magnesium; sodium perchlorate; water; instrumentation; Mars; Martian atmosphere; radar; subglacial environment; Article; astronomy; cosmological phenomena; dielectric constant; electromagnetic radiation; electromagnetism; environmental temperature; physical chemistry; priority journal; quantitative analysis; radiation detection; radiation measurement; radiofrequency; sound intensity; south solar layered deposit; space flight; subglacial liquid water; surface property; velocity |
语种 | 英语 |
来源期刊 | Science
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/244953 |
作者单位 | Istituto di Radioastronomia, Istituto Nazionale di Astrofisica, Via Piero Gobetti 101, Bologna, 40129, Italy; Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, Via della Vasca Navale 84, Roma, 00146, Italy; Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica, Via del Fosso del Cavaliere 100, Roma, 00133, Italy; Agenzia Spaziale Italiana, Via del Politecnico, Roma, 00133, Italy; Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica, Vicolo Osservatorio 5, Padova, 35122, Italy; Consiglio Nazionale delle Ricerche, Istituto per il Rilevamento Elettromagnetico dell’Ambiente, Via Diocleziano 328, Napoli, 80124, Italy; Dipartimento di Ingegneria dell’Informazione, Elettronica e Telecomunicazioni, Università degli Studi di Roma “La Sapienza,”, Via Eudossiana 18, Roma, 00184, Italy; E.P. Elettronica Progetti, Via Traspontina 25, Ariccia, RM 00040, Italy; International Research School of Planetary Sciences, Università degli Studi “Gabriele d’Annunz... |
推荐引用方式 GB/T 7714 | Orosei R.,Lauro S.E.,Pettinelli E.,et al. Radar evidence of subglacial liquid water on Mars[J],2018,361(6401). |
APA | Orosei R..,Lauro S.E..,Pettinelli E..,Cicchetti A..,Coradini M..,...&Seu R..(2018).Radar evidence of subglacial liquid water on Mars.Science,361(6401). |
MLA | Orosei R.,et al."Radar evidence of subglacial liquid water on Mars".Science 361.6401(2018). |
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