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相关概念视频

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...
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,...
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...
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.
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Sulfur Assimilation01:20

Sulfur Assimilation

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相关实验视频

Updated: Jun 18, 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

最热的星球 最热的星球

Joseph Harrington1, Statia Luszcz, Sara Seager

  • 1Department of Physics, University of Central Florida, Orlando, Florida 32816-2385, USA. jharring@physics.ucf.edu

Nature
|May 15, 2007
PubMed
概括
此摘要是机器生成的。

来自最小的过境系外行星HD 149026b的直接检测到的热辐射揭示了令人惊的高温. 这一发现挑战了标准的系外行星大气模型,并表明了独特的热特性.

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相关实验视频

Last Updated: Jun 18, 2026

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

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Published on: November 16, 2013

Scattering And Absorption of Light in Planetary Regoliths
11:34

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科学领域:

  • 外系行星科学 外系行星科学
  • 天体物理学 天体物理学
  • 行星大气层的行星大气层

背景情况:

  • 已知有200多个太阳系外行星,但只有14个显示过境几何.
  • 穿越系外行星允许直接测量行星属性.
  • 之前对系外行星的热辐射研究与假设邦德白度为~0.3.3的预测一致.

研究的目的:

  • 报告从HD 149026b直接检测到的热辐射,这是已知的最小的过境系外行星.
  • 为了研究HD 149026b的热特性和大气特征.
  • 将观察到的热辐射与理论模型进行比较.

主要方法:

  • 来自系外行星HD 149026b的热辐射在8微米处的直接检测.
  • 测量亮度温度的方法.
  • 将观察到的数据与黑体排放模型和不同的白度场景进行比较.

主要成果:

  • 从HD 149026b.直接检测热辐射的热辐射.
  • 测得的亮度温度为2,300 ± 200 K,距离8微米.
  • 观察到的温度明显高于标准模型预测的温度,其非零色白度.

结论:

  • 标准统一的黑体模型具有非零的白度与观察到的数据不一致.
  • 高温可能意味着极低的白度,强烈的8微米辐射,时间变化或替代热源.
  • 一个即时再发射黑体模型与数据保持一致,表明了新的大气特性,可能是由于重元素的丰富.