Open Dataset
Data Structure ?
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Data Structure ?
*The above analysis is the result extracted and analyzed by the system, and the specific actual data shall prevail.
README.md
私たちが住む太陽系外の惑星を初めて目にしたのは1992年で、その時、いくつかの地球質量の惑星がパルサーPSR B1257+12を周回していることが検出されました。このデータセットでは、あなたもすべての発見された太陽系外惑星(火星、土星、さらには地球のようなおなじみの惑星も含む)の特性を分析することで宇宙探検家になることができます。データフィールドには、**惑星**と**母星の属性**、**発見方法**、そして(もちろん)**発見日**が含まれます。
データはもともと[ハンノ・ライン][1]によって収集され、[Open Exoplanet CatalogueのGitHubリポジトリ][2]で更新が続けられています。もしあなたが新しい太陽系外惑星を発見した場合は、そこにプルリクエストを送信してください。
## 定数
- **木星質量**:1.8991766e+27 kg
- **太陽質量**:1.9891e+30 kg
- **木星半径**:69911000 m
- **太陽半径**:6.96e+08 m
## ライセンス
このデータベースはMITライセンスの下で提供されています。科学論文で使用する場合は、[GitHub上のOpen Exoplanet Catalogue][3]または[このarXiv論文][4]への引用を含めてください。
[1]: https://github.com/hannorein "ハンノ・ライン"
[2]: https://github.com/OpenExoplanetCatalogue/open_exoplanet_catalogue
[3]: https://github.com/OpenExoplanetCatalogue/open_exoplanet_catalogue
[4]: http://arxiv.org/abs/1211.7121
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