関連する実験動画
Updated: Jun 10, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
ガリレオとケプラー以来,惑星科学の400年
1Department of Astronomy and College of Engineering, 328 Space Sciences Building, Cornell University, Ithaca, New York 14853-6801, USA. jab16@cornell.edu
Nature
|July 31, 2010
まとめ
過去50年にわたる宇宙船の探査は,太陽系の理解に革命を起こし,多様な天体と活発なプロセスを明らかにしました. この新しい知識は,起源モデルをテストし,地球外生命の探求を可能にします.
科学分野:
- 惑星科学 惑星科学
- 天文学 天文学
- 天体生物学 アストロバイオロジー
背景:
- 何世紀もの間,地上の望遠鏡とモデルは,太陽系に関する知識を定義してきました.
- ここ数十年,宇宙船による変化を起こすインシット探査が行われている.
研究 の 目的:
- 宇宙船のミッションが太陽系を理解する上で与える影響を強調する.
- 惑星科学と起源論の進化を強調する.
- 地球外生命の探求と将来の研究方向性を強調する.
主な方法:
- 歴史的な天文観測のレビュー.
- 数十年にわたる宇宙ミッションからのデータの分析.
- 現在の惑星科学知識の統合.
主要な成果:
- 宇宙船は,太陽系の膨大な多様性とダイナミックなプロセスを明らかにしました.
- 惑星や衛星を形作る暴力的な歴史的出来事の証拠.
- 太陽系起源のテスト可能なモデルの開発.
結論:
- 宇宙船の探査は,惑星科学を根本的に進歩させた.
- 現在の知識は,潜在的な地球外生命の生息地を探索することをサポートしています.
- 将来の研究には,系外惑星を含む,標的を絞った研究が必要です.
関連する概念動画
Kepler's Third Law of Planetary Motion
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. In 1909, he formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe. However, in 1918, he published his third law of planetary motion, which gives a precise mathematical relationship between a planet's average distance from the Sun and the amount of time it takes to revolve around the Sun. It...
Kepler's First Law of Planetary Motion
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Kepler's Second Law of Planetary Motion
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
Space-Time Curvature and the General Theory of Relativity
In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...
Gravitation
In the years before Newton, a general belief prevailed that different laws governed objects in the sky than objects on Earth. When Kepler wrote down the three laws of planetary motion, explaining in detail the geometrical properties of the planetary orbits around the Sun, there was no immediate idea to discern their connection with more fundamental laws. It was Isaac Newton who, in 1665–66, figured out the connection between planetary motion, the motion of the moon around the Earth, and the...
Circular Orbits and Critical Velocity for Satellites
The Moon orbits around the Earth. In turn, the Earth (and other planets) orbit the Sun. The space directly above our atmosphere is filled with artificial satellites in orbit. One can examine the circular orbit, the simplest kind of orbit, to understand the relationship between the speed and the period of planets and satellites with respect to their positions and the bodies that they orbit.
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...

