Bilingual edition: English is preserved and Chinese follows each unit. Terminology uses the confirmed v20260916 glossary; automated semantic review remains traceable.
中英双语版:英文原文完整保留,中文紧随对应单元;术语采用 v20260916 确认表,自动语义审校结果可追溯。

The Kepler Satellite

开普勒卫星

NASA Image

"The Kepler Mission was specifically designed to survey our region of the Milky Way galaxy to discover hundreds of Earth-size and smaller planets in or near the habitable zone and determine the fraction of the hundreds of billions of stars in our galaxy that might have such planets."

开普勒任务专门设计用于调查银河系我们的区域,以发现数百颗类似地球大小或更小的行星,这些行星位于或接近宜居带,从而确定银河系中数百亿颗恒星中可能拥有此类行星的比例。

"The scientific objective of the Kepler Mission was to explore the structure and diversity of planetary systems. This is achieved by surveying a large sample of stars to:

  • Determine the percentage of terrestrial and larger planets that are in or near the habitable zone of a wide variety of stars
    确定宽种类恒星的适居带中或附近的大气行星和类地行星的百分比
  • Determine the distribution of sizes and shapes of the orbits of these planets
    确定这些行星轨道的大小和形状分布
  • Estimate how many planets there are in multiple-star systems
    估算多重星系中行星的数量
  • Determine the variety of orbit sizes and planet reflectivities, sizes, masses and densities of short-period giant planets
    确定短周期巨行星的轨道大小、行星反照率、大小、质量和密度的多样性
  • Identify additional members of each discovered planetary system using other techniques
    使用其他技术识别每个发现的行星系统中的其他成员
  • Determine the properties of those stars that harbor planetary systems."
    确定拥有行星系统的恒星的特性。
开普勒任务的科学目标是探索行星系统的结构和多样性。这通过调查大量恒星样本来实现:

Kepler primarily used the transit method for detecting extrasolar planets. Kepler found planets by looking for tiny dips in the brightness of a star when a planet crosses in front of it - we say the planet transits the star. Once detected, the planet's orbital size can be calculated from the period and the mass of the star using Kepler's Third Law of planetary motion. The size of the planet is found from the depth of the transit (how much the brightness of the star drops) and the size of the star. From the orbital size and the temperature of the star, the planet's characteristic temperature can be calculated. From this the question of whether or not the planet is habitable (not necessarily inhabited) can be answered.

开普勒主要使用凌星法来探测系外行星。开普勒通过观察当行星掠过恒星前方时,恒星亮度的微小下降来发现行星——我们说行星凌星。一旦发现行星,可以利用行星的轨道周期和恒星的质量,通过开普勒第三定律计算出行星的轨道半径。行星的大小可以从凌星的深度(恒星亮度下降的程度)和恒星的大小来确定。从轨道半径和恒星的温度,可以计算出行星的特征温度。由此可以判断该行星是否宜居(不一定是被居住)。

Launched on March 7, 2009, the Kepler satellite discovered more than 2,600 planets. The spacecraft was retired in a safe orbit on October 30, 2018. The role of hunting planets was transferred to the TESS satellite. Kepler took more data than could be immediately analyzed, so discoveries from that data were made years after the cessation of the mission. One of those discoveries was the planet Kepler-1649c orbiting around its host red dwarf star. This newly discovered exoplanet is in its star's habitable zone and is the closest to Earth in size and temperature found yet in Kepler's data.

2009年3月7日发射的开普勒卫星发现了超过2,600颗行星。该航天器于2018年10月30日安全进入轨道退役。寻找行星的任务转由TESS卫星承担。由于开普勒收集的数据量超过了当时分析能力,因此从这些数据中发现的成果是在任务结束后数年才公布的。其中一项发现是开普勒-1649c行星,它围绕着其红矮星宿主恒星运行。这颗新发现的系外行星位于其恒星的宜居带内,并且在开普勒的数据中,是迄今为止在大小和温度方面最接近地球的发现。
NASA 图像
Index

References
Satellite Instruments

Kepler, NASA

Kepler 1649c
索引参考卫星仪器 开普勒,NASA 开普勒 1649c
 
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Kepler Planetary Discoveries

开普勒行星发现

NASA Image

Kepler discovered more than 2,600 planets. The spacecraft was retired in a safe orbit on October 30, 2018. The role of hunting planets was transferred to the TESS satellite. Kepler took more data than could be immediately analyzed, so discoveries from that data were made years after the cessation of the mission. One of those discoveries was the planet Kepler-1649c orbiting around its host red dwarf star. This newly discovered exoplanet is in its star's habitable zone and is the closest to Earth in size and temperature found yet in Kepler's data.

开普勒发现了超过2600颗行星。航天器于2018年10月30日安全进入轨道退役。寻找行星的任务转由TESS卫星承担。由于开普勒收集的数据量超过当时分析能力,因此从这些数据中发现的成果是在任务结束后几年才公布的。其中一项发现是开普勒-1649c行星,它围绕其红矮星运行。这颗新发现的系外行星位于其恒星的宜居带内,并且是迄今为止在开普勒数据中发现的、在大小和温度上最接近地球的行星。
NASA 图像
Index

References
Satellite Instruments

Kepler, NASA

Kepler 1649c
索引参考卫星仪器 开普勒,NASA 开普勒 1649c
 
HyperPhysics********** Astrophysics
HyperPhysics ********** 天体物理学
R Nave
Go Back
返回