파일:PIA22095-TRAPPIST-1-SolarSystemComparison-20180205.jpg
이 파일은 위키미디어 공용에 있으며, 다른 프로젝트에서 사용하고 있을 가능성이 있습니다. 해당 파일에 대한 설명이 아래에 나와 있습니다.
파일 설명
| 설명PIA22095-TRAPPIST-1-SolarSystemComparison-20180205.jpg |
English: PIA22095: Comparing TRAPPIST-1 to the Solar System
https://photojournal.jpl.nasa.gov/catalog/PIA22095 This graph presents known properties of the seven TRAPPIST-1 exoplanets (labeled b through h), showing how they stack up to the inner rocky worlds in our own solar system. The horizontal axis shows the level of illumination that each planet receives from its host star. TRAPPIST-1 is a mere 9 percent the mass of our Sun, and its temperature is much cooler. But because the TRAPPIST-1 planets orbit so closely to their star, they receive comparable levels of light and heat to Earth and its neighboring planets. The vertical axis shows the densities of the planets. Density, calculated based on a planet's mass and volume, is the first important step in understanding a planet's composition. The plot shows that the TRAPPIST-1 planet densities range from being similar to Earth and Venus at the upper end, down to values comparable to Mars at the lower end. The relative sizes of the planets are indicated by the circles. The masses and densities of the TRAPPIST-1 planets were determined by careful measurements of slight variations in the timings of their orbits using extensive observations made by NASA's Spitzer and Kepler space telescopes, in combination with data from Hubble and a number of ground-based telescopes. These measurements are the most precise to date for any system of exoplanets. By comparing these measurements with theoretical models of how planets form and evolve, researchers have determined that they are all rocky in overall composition. Estimates suggest the lower-density planets could have large quantities of water -- as much as 5 percent by mass for TRAPPIST-1d. Earth, in comparison, has only about 0.02 percent of its mass in the form of water. NASA's Jet Propulsion Laboratory, Pasadena, California, manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at Caltech, also in Pasadena. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at Caltech/IPAC. Caltech manages JPL for NASA. For additional information about the Spitzer mission, visit http://www.nasa.gov/spitzer and http://spitzer.caltech.edu. For additional information on the Kepler and the K2 mission, visit www.nasa.gov/Kepler. For additional information about exoplanets, visit https://exoplanets.nasa.gov/. |
| 날짜 | |
| 출처 | https://photojournal.jpl.nasa.gov/jpeg/PIA22095.jpg |
| 저자 | NASA/JPL-Caltech |
라이선스
| 이 파일의 저작권자인 NASA/JPL-Caltech은 저작권자를 명시하는 조건에 따라 누구에게나 어떤 목적으로든지 제한 없이 사용할 수 있도록 허용하였습니다. 재배포나 이차적 저작물 작성 및 상업적 이용 등이 허용됩니다. | |
|
Attribution |
| According to JPL's image use policy additional restriction is that no endorsement of any product or service by Caltech, JPL or NASA is claimed or implied.
Caltech's disclaimer: Caltech makes no representations or warranties with respect to ownership of copyrights in the images, and does not represent others who may claim to be authors or owners of copyright of any of the images, and makes no warranties as to the quality of the images. Caltech shall not be responsible for any loss or expenses resulting from the use of the images, and you release and hold Caltech harmless from all liability arising from such use. Usage on the English Wikipedia: On the English Wikipedia you can use the {{JPL Image}} template to display the copyright notice. (See w:Wikipedia:Using JPL images for details) |
설명
이 파일에 묘사된 항목
다음을 묘사함
5 2 2018
파일 역사
날짜/시간 링크를 클릭하면 해당 시간의 파일을 볼 수 있습니다.
| 날짜/시간 | 섬네일 | 크기 | 사용자 | 설명 | |
|---|---|---|---|---|---|
| 현재 | 2018년 2월 6일 (화) 17:53 | 4,800 × 2,700 (578 KB) | wikimediacommons>Drbogdan | User created page with UploadWizard |
이 파일을 사용하는 문서
다음 문서 1개가 이 파일을 사용하고 있습니다: