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相关论文: Mars Before the Space Age

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Mars is the Solar System's canonical small, rocky planet that transitioned from early geologic activity and surface liquid water to a cold and arid planet with a thin, cold, CO$_2$-dominated atmosphere. The evolution of Mars, in the context…

Gillevinia straata, the scientific name [1, 2] recognizing the first extraterrestrial living form ever nomenclated, as well as the existence of a new biological kingdom, Jakobia, in a new biosphere -Marciana- of what now has become the…

综合物理 · 物理学 2007-06-16 Gilbert V. Levin

The Red Planet has fascinated humans for millennia, especially for the last few centuries, and particularly during the Space Age. The nagging suspicion of extant Martian life is both fed by, and drives the many space missions to Mars and…

天体物理仪器与方法 · 物理学 2020-08-14 Robert Hunt

Despite great advances in our understanding of the formation of the Solar System, the evolution of the Earth, and the chemical basis for life, we are not much closer than the ancient Greeks to an answer of whether life has arisen and…

天体物理学 · 物理学 2007-05-23 Eric Gaidos , Franck Selsis

Mars' tadpole craters are small, young craters whose crater rims are incised by one or more exit breaches but lack visible inlets. The tadpole forming climate records the poorly understood drying of Mars since the Early Hesperian. A third…

地球与行星天体物理 · 物理学 2024-07-17 Alexandra O. Warren , Sharon A. Wilson , Alan Howard , Axel Noblet , Edwin S. Kite

The detection of geologically recent channels at the end of the twentieth century rapidly suggested that liquid water could have been present on Mars up to recent times. A mechanism involving melting of water ice during ice ages in the last…

地球与行星天体物理 · 物理学 2015-12-17 Mathieu Vincendon

In 1953 I heard of an experiment in 1925 by Bengt Str\"omgren where he observed transit times with the meridian circle at the Copenhagen University Observatory measuring the current in a photocell behind slits when a star was crossing. In…

天体物理仪器与方法 · 物理学 2024-04-23 Erik Høg

It is currently uncertain as to whether methane exists on Mars. Data from the Curiosity Rover suggests a background methane concentration of a few tenths parts per billion whereas data from the Trace Gas Orbiter suggest an upper limit of…

In the late 1620s the Neapolitan telescope maker Francesco Fontana was the first to observe the sky using a telescope with two convex lenses, which he had manufactured himself. Fontana succeeded in drawing the most accurate maps of the…

物理学史与哲学 · 物理学 2017-04-20 Paolo Molaro

The Solar System includes two planets --- Mercury and Mars --- significantly less massive than Earth, and all evidence indicates that planets of similar size orbit many stars. In fact, one of the first exoplanets to be discovered is a…

地球与行星天体物理 · 物理学 2015-06-17 E. Sinukoff , B. Fulton , L. Scuderi , E. Gaidos

The decay of the martian atmosphere - which is dominated by carbon dioxide - is a component of the long-term environmental change on Mars from a climate that once allowed rivers to flow to the cold and dry conditions of today. The minimum…

地球与行星天体物理 · 物理学 2017-12-12 Edwin S. Kite , Jean-Pierre Williams , Antoine Lucas , Oded Aharonson

The long term dreams to approach Mars requires numerous spacecraft attempts for exploration as well as to understand the perception of the red planet. Before launching a mission, the space probe undergoes critical ground testing and…

天体物理仪器与方法 · 物理学 2021-04-07 Malaya Kumar Biswal M , Ramesh Naidu Annavarapu

An origin of Earth life on Mars would resolve significant inconsistencies between the inferred history of life and Earth's geologic history. Life as we know it utilizes amino acids, nucleic acids, and lipids for the metabolic,…

地球与行星天体物理 · 物理学 2022-07-20 Christopher E. Carr

All three terrestrial planets with atmospheres support O3 layers of some thickness. While currently only that of Earth is substantial enough to be climatically significant, we hypothesize that ancient Mars may also have supported a thick O3…

地球与行星天体物理 · 物理学 2013-03-18 Justin Deighan , Robert E Johnson

The frequently discovered flooding structure on Mars and other planets has long been an intriguing mystery remained un-disclosed so far. Considering that on Earth, quite a few low melting point liquid metals or their alloy can be candidates…

综合物理 · 物理学 2014-03-18 Jing Liu , Yunxia Gao , Huangde Li

Ancient hydrology is recorded by sedimentary rocks on Mars. The most voluminous sedimentary rocks that formed during Mars' Hesperian period are sulfate-rich rocks, explored by the $Opportunity$ rover from 2004-2012 and soon to be…

地球与行星天体物理 · 物理学 2019-08-14 Edwin S. Kite , Mohit Melwani Daswani

For decades, scientists have tried to explain the evidence for fluvial activity on early Mars, but a consensus has yet to emerge regarding the mechanism for producing it. One hypothesis suggests early Mars was warmed by a thick greenhouse…

地球与行星天体物理 · 物理学 2016-11-21 Natasha E. Batalha , Ravi K. Kopparapu , Jacob Haqq-Misra , James F. Kasting

Recent discoveries imply that Early Mars was habitable for life-as-we-know-it; that Enceladus might be habitable; and that many stars have Earth-sized exoplanets whose insolation favors surface liquid water. These exciting discoveries make…

地球与行星天体物理 · 物理学 2018-08-08 Edwin S. Kite , Eric Gaidos , Tullis C. Onstott

The climate of Mars likely evolved from a warmer, wetter early state to the cold, arid current state. However, no solutions for this evolution have previously been found to satisfy the observed geological features and isotopic measurements…

地球与行星天体物理 · 物理学 2015-12-03 Renyu Hu , David M. Kass , Bethany L. Ehlmann , Yuk L. Yung