
火星在数十亿年前曾拥有活跃的火山活动、磁场(magnetic field)和液态水。由于体积较小,其内部冷却速度远快于地球(Earth),导致了地质活动的停止。最新的研究探讨了火星目前内部的热状态。
The planet Mars is a cold and dry world completely devoid of life, but billions of years ago things were much different. This is when Mars had a much warmer interior than it does today, resulting in active volcanism that replenished its atmosphere, a magnetic field that protected the planet from harmful solar and cosmic radiation, and a surface of flowing liquid water. But due to Mars’s small size, the interior cooled far faster than Earth’s has cooled, leading to a loss of volcanism, near-absolute depletion of its magnetic field, and complete evaporation of all surface liquid water. But what is the interior heat of Mars like today?
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本站仅展示标题与摘要,正文版权归原作者及原发布机构所有。 原作者:Laurence Tognetti, MSc (https://www.universetoday.com/authors/laurencetognetti)。 原始页面