在可见波长的海王星云结构.

H B Hammel

Science (New York, N.Y.)

|June 9, 1989

概括

1988年,数字图像揭示了海王星上一个明亮的特征,可以在甲吸收带中看到. 这一发现对于理解海王星至关重要.

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Endogenous CO<sub>2</sub> ice mixture on the surface of Europa and no detection of plume activity.

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在可见波长的海王星云结构.

科学领域:

背景情况:

研究的目的:

主要方法:

相关概念视频

相关文章

Endogenous CO<sub>2</sub> ice mixture on the surface of Europa and no detection of plume activity.

Worlds beyond: A strategy for the detection and characterization of exoplanets. Executive summary of a report of the ExoPlanet Task Force Astronomy and Astrophysics Advisory Committee Washington, DC June 23, 2008.

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Hubble Space Telescope Imaging of Neptune's Cloud Structure in 1994.

HST imaging of atmospheric phenomena created by the impact of comet Shoemaker-Levy 9.

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相关实验视频

在可见波长的海王星云结构.

科学领域:

背景情况:

研究的目的:

主要方法:

相关概念视频

相关文章

Endogenous CO<sub>2</sub> ice mixture on the surface of Europa and no detection of plume activity.

Worlds beyond: A strategy for the detection and characterization of exoplanets. Executive summary of a report of the ExoPlanet Task Force Astronomy and Astrophysics Advisory Committee Washington, DC June 23, 2008.

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Hubble Space Telescope Imaging of Neptune's Cloud Structure in 1994.

HST imaging of atmospheric phenomena created by the impact of comet Shoemaker-Levy 9.

Impact debris particles in Jupiter's stratosphere.

主要成果:

结论: