Jove
Visualize
お問い合わせ
JoVE
x logofacebook logolinkedin logoyoutube logo
JoVEについて
概要リーダーシップブログJoVEヘルプセンター
著者向け
出版プロセス編集委員会範囲と方針査読よくある質問投稿
図書館員向け
推薦の声購読アクセスリソース図書館諮問委員会よくある質問
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experimentsアーカイブ
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教員リソースセンター教員サイト
利用規約
プライバシーポリシー
ポリシー

関連する概念動画

States of Water01:23

States of Water

Water exists in any one of the three classical states: solid (ice), liquid (water), and gas (steam or water vapor). The state of water depends on i) the intermolecular forces that draw molecules together and ii) the kinetic energy that leads to movements that pull them apart.
Water freezes when the intermolecular forces are greater than the kinetic energy. Unlike most other substances, water is less dense in its solid state than in its liquid state. This is because each water molecule can form...
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Rocket Propulsion in Empty Space - I01:13

Rocket Propulsion in Empty Space - I

The driving force for the motion of any vehicle is friction, but in the case of rocket propulsion in space, the friction force is not present. The motion of a rocket changes its velocity (and hence its momentum) by ejecting burned fuel gases, thus causing it to accelerate in the direction opposite to the velocity of the ejected fuel. In this situation, the mass and velocity of the rocket constantly change along with the total mass of ejected gases. Due to conservation of momentum, the rocket's...
Rocket Propulsion in Gravitational Field - II01:03

Rocket Propulsion in Gravitational Field - II

A rocket's velocity in the presence of a gravitational field is decreased by the amount of force exerted by Earth's gravitational field, which opposes the motion of the rocket. If we consider thrust, that is, the force exerted on a rocket by the exhaust gases, then a rocket's thrust is greater in outer space than in the atmosphere or on a launch pad. In fact, gases are easier to expel in a vacuum.
A rocket's acceleration depends on three major factors, consistent with the equation for the...
Acceleration due to Gravity on Other Planets01:24

Acceleration due to Gravity on Other Planets

The gravitational acceleration of an object near the Earth's surface is called the acceleration due to gravity. It can be measured by conducting simple experiments on Earth. However, such an experiment is impossible to conduct on the surface of other planets.
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...

こちらも読む

関連記事

共著者、ジャーナル、引用グラフによってこの研究に関連する記事。

並び替え
Same author

Comparison between ozone column depths and methane lifetimes computed by one- and three-dimensional models at different atmospheric O<sub>2</sub> levels.

Royal Society open science·2023
Same author

Novel Antarctic yeast adapts to cold by switching energy metabolism and increasing small RNA synthesis.

The ISME journal·2021
Same author

Controls on the Archean climate system investigated with a global climate model.

Astrobiology·2014
Same author

Reaching 1 m deep on Mars: the Icebreaker drill.

Astrobiology·2013
Same author

The cryptoendolithic microbial environment in the Ross Desert of Antarctica: Mathematical models of the thermal regime.

Microbial ecology·2013
Same author

The cryptoendolithic microbial environment in the Ross Desert of Antarctica: Light in the photosynthetically active region.

Microbial ecology·2013
Same journal

Incoming US science academy chief vows to 'double down' on research.

Nature·2026
Same journal

Author Correction: Synthesis of enantioenriched atropisomers by biocatalytic deracemization.

Nature·2026
Same journal

Electrodeposited self-assembled molecules for perovskite photovoltaics.

Nature·2026
Same journal

Neutrino's nursery found: the 'Shadow Blaster'.

Nature·2026
Same journal

Dementia risk in middle-aged people linked to a blood protein.

Nature·2026
Same journal

Daily briefing: What's really happening with trust in science.

Nature·2026
関連記事をすべて見る

関連する実験動画

Updated: Jun 29, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 16, 2013

火星を居住可能にする.

C P McKay1, O B Toon, J F Kasting

  • 1Space Science Division, NASA Ames Research Center, Moffett Field, California 94035, USA.

Nature
|August 8, 1991
PubMed
まとめ
この要約は機械生成です。

火星は,居住のためにテラフォームされるかもしれない. 成功は,植物と人間の生活を支えるために,地球上で容易に利用可能な二酸化炭素,水,窒素に依存しています.

キーワード:
NASA Center ARCは,NASAセンターのARCとして運営されています.NASAの規律 エクゾバイオロジーNASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASAの規律番号52-80は,NASA エクゾバイオロジープログラム非NASAのセンターです.

さらに関連する動画

Conducting Miller-Urey Experiments
11:10

Conducting Miller-Urey Experiments

Published on: January 21, 2014

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

関連する実験動画

Last Updated: Jun 29, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 16, 2013

Conducting Miller-Urey Experiments
11:10

Conducting Miller-Urey Experiments

Published on: January 21, 2014

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

科学分野:

  • 惑星科学は惑星科学である.
  • 天体生物学 アストロバイオロジー

背景:

  • 現在の理解では,火星は生命が存在しないことを示唆しています.
  • 火星のテラフォーミングは,地球外生命の居住のための潜在的な経路を示しています.

研究 の 目的:

  • 火星を居住可能な惑星に変換する可能性を評価するためです.
  • 火星の居住可能性のための重要な材料要件を特定する.

主な方法:

  • 火星の地質学的物質の分析.
  • 大気や地下資源の利用可能性の評価.

主要な成果:

  • 居住可能性の鍵となる要素 (二酸化炭素,水,窒素) は極めて重要です.
  • これらの材料の豊富さ,分布,形状は,重要な要因です.

結論:

  • 火星を居住可能にするのは理論的には可能だ.
  • 重要な資源の利用可能性は,地形改造の成功を左右する.