相关实验视频
Updated: Mar 21, 2026

06:48
Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
Published on: May 10, 2020
4.0K
温和的地球大小的行星穿过附近的超冷矮星
Michaël Gillon1, Emmanuël Jehin1, Susan M Lederer2
1Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août 19C, 4000 Liège, Belgium.
Nature
|May 3, 2016
概括
天文学家发现了三颗地球大小的系外行星围绕一颗极冷的矮星运行. 这些行星靠近恒星
科学领域:
- 天文学与天体物理学
- 外行星科学
- 恒星进化
背景情况:
- 超冷矮星是恒星般的天体, 温度低于2700K.
- 它们占太阳附近天文物体的15%,包括低质量恒星和棕矮星.
- 核心积聚理论预测这些天体周围有大量的陆地行星.
研究的目的:
- 为了寻找和描述围绕极冷矮星运行的地球行星.
- 在低质量恒星周围测试行星形成理论.
- 在超冷矮星的可居住区域研究行星的潜在可居住性.
主要方法:
- 观测天文学利用过境光度检测系外行星.
- 分析主体超冷矮星的红外亮度和大小.
- 确定行星辐射水平的恒星特征.
主要成果:
- 发现三颗地球大小的行星在距离我们12个帕塞克的极冷矮星上运行.
- 内部行星收到4倍和2倍的地球辐射,靠近可居住区的内部边缘.
- 第三个行星的辐射可能低于地球,有11个可能的轨道.
结论:
- 这一发现证实了超冷矮星周围的陆地行星存在.
- 附近的系统为详细的系外行星大气表征提供了独特的机会.
- 在寻找潜在可居住系外行星的过程中,
相关概念视频
Kepler's First Law of Planetary Motion
6.0K
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,...
6.0K
Kepler's Third Law of Planetary Motion
4.5K
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...
4.5K
Kepler's Second Law of Planetary Motion
5.7K
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...
5.7K
Schwarzschild Radius and Event Horizon
2.9K
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...
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...
2.9K
Conditions on Early Earth
103.0K
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.
103.0K
Conditions on Early Earth
2.9K
2.9K

