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相关概念视频

Kepler's Second Law of Planetary Motion01:29

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...
Kepler's Third Law of Planetary Motion01:18

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 Motion01:10

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,...
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
Subatomic Particles03:37

Subatomic Particles

Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
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...

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相关实验视频

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Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
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一个子水星大小的系外行星.

Thomas Barclay1, Jason F Rowe, Jack J Lissauer

  • 1NASA Ames Research Center, Moffett Field, California 94035, USA. thomas.barclay@nasa.gov

Nature
|February 22, 2013
PubMed
概括

天文学家发现了开普勒-37b,这是迄今为止发现的最小的系外行星,比水星小得多. 这个小的,可能是岩石的世界围绕一颗类似太阳的恒星运行,为行星系统的多样性提供了新的见解.

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Last Updated: May 14, 2026

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Published on: May 10, 2020

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10:35

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科学领域:

  • 外行星科学是外行星的科学.
  • 比較行星學 比較行星學

背景情况:

  • 外行星的发现揭示了不同的行星系统,不像我们自己的.
  • 最近的进展允许探测地球大小和较小的系外行星.
  • 以前,没有发现比我们太阳系中更小的系外行星.

研究的目的:

  • 报告发现了一个远小于水星的系外行星.
  • 描述迄今为止发现的最小系外行星及其宿主恒星.

主要方法:

  • 使用开普勒太空望远镜的运输光度数据.
  • 分析光曲线变化以确定行星大小和轨道参数.

主要成果:

  • 发现开普勒-37b,一个比水星小的系外行星,与月球大小相提并论.
  • 开普勒-37b是围绕类似太阳的恒星开普勒-37旋转的三个行星中最内在的.
  • 这颗行星的小尺寸和距离恒星的近距离表明,它可能是岩石组成的,没有大气或水.

结论:

  • 开普勒-37b代表了新发现的系外行星大小的下限.
  • 这一发现突显了其他恒星系统中行星天体的巨大多样性.
  • 进一步研究这样的小型系外行星对于理解行星的形成和进化至关重要.