可住帶

可住帶（宜居帶，適居帶，英文：circumstellar habitable zone，Goldilocks zone, CHZ），就係喺圍繞恆星軌道嘅範圍，而裏頭嘅行星表面有足夠大氣壓力同有液態水^[1]^[2]。亦即係喺天文學指行星系之中適合生命存在嘅區域。CHZ 嘅範圍係基於嗰個星球嘅同佢太陽嘅距離，同埋埋接收嘅輻射能量。由於液態水對地球生物圈好重要，CHZ 同埋裏頭星體嘅特質，會影響發展生命，同埋出現類似地球生物嘅可能^[3]。

睇埋

攷

↑ Kopparapu, Ravi Kumar (2013). "A revised estimate of the occurrence rate of terrestrial planets in the habitable zones around kepler m-dwarfs". The Astrophysical Journal Letters. 767 (1): L8. arXiv:1303.2649. Bibcode:2013ApJ...767L...8K. doi:10.1088/2041-8205/767/1/L8.
↑ Cruz, Maria; Coontz, Robert (2013). "Exoplanets - Introduction to Special Issue". Science. 340 (6132): 565. doi:10.1126/science.340.6132.565. 喺18 May 2013搵到.
↑ "VPL Glossary".

[kopparapu-2013-1] Kopparapu, Ravi Kumar (2013). "A revised estimate of the occurrence rate of terrestrial planets in the habitable zones around kepler m-dwarfs". The Astrophysical Journal Letters. 767 (1): L8. arXiv:1303.2649. Bibcode:2013ApJ...767L...8K. doi:10.1088/2041-8205/767/1/L8.

[SCI-20130503-2] Cruz, Maria; Coontz, Robert (2013). "Exoplanets - Introduction to Special Issue". Science. 340 (6132): 565. doi:10.1126/science.340.6132.565. 喺18 May 2013搵到.

[3] "VPL Glossary".

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