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外惑星

8 件の記事

The amount of water vapor in Earth's atmosphere has risen over recent decades,[1] making heavy rainfall events more severe.[2]

水蒸気の科学地球の気候変動と宇宙における役割

水蒸気温室効果ガス湿度気候変動
The atmospheric gases around Earth scatter blue light (shorter wavelengths) more than light toward the red end (longer wavelengths) of the visible spectrum; thus, a blue glow over the horizon is seen when observing Earth from outer space. The Moon is visible in the background.

惑星の大気宇宙のガス層が形成される仕組みと多様な組成

惑星大気天文学大気組成太陽系
In the Vertical Processing Facility (VPF), Galileo is prepared for mating with the Inertial Upper Stage booster.

ガリレオ計画木星とその衛星を解き明かした歴史的探査機

ガリレオ探査機木星探査NASA大気圏突入プローブ
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惑星の分類内惑星と外惑星の違いとは

惑星内惑星外惑星地球
An angle ε is drawn between two straight lines from Earth to the Sun, and from Earth to the planet. This is demonstrated for different positions along circular orbits, both for planets closer to the Sun (where the angle is always less than 90°), and for outer planets (for which the angle can range from 0° to 180°), while distinguishing east and west sides.

離角(elongation)とは?天文学における惑星と太陽の角度的な距離を解説

離角最大離角内惑星外惑星
The evolution of the apparent diameter and phases of Venus

惑星の位相地球から見た惑星の満ち欠けの仕組み

惑星位相内惑星外惑星
In the Vertical Processing Facility (VPF), Galileo is prepared for mating with the Inertial Upper Stage booster.

ガリレオ宇宙探査機木星の謎に迫ったNASAの壮大なミッション

ガリレオ探査機木星探査NASA大気探査機
The atmospheric gases around Earth scatter blue light (shorter wavelengths) more than light toward the red end (longer wavelengths) of the visible spectrum; thus, a blue glow over the horizon is seen when observing Earth from outer space. The Moon is visible in the background.

惑星大気のメカニズム組成から構造、宇宙への散逸まで

惑星大気天文学大気組成外惑星