行星科学深探 Astronomy

8 个科学问题 · 天文 Astronomy

本页目录

柯伊伯带与奥尔特云在结构、距离和起源上有何本质区别?

What are the essential differences in structure, distance, and origin between the Kuiper Belt and the Oort Cloud?

柯伊伯带是位于海王星轨道外约 30–50 天文单位的盘状区域,由冰质天体构成、基本处于行星形成后原位保留的状态。奥尔特云则是延伸至数千至十万天文单位的球壳,被认为是早期太阳系外围天体被巨行星引力散射到遥远轨道后形成的彗星储库,二者一扁一盘、一远一球,起源机制迥异。
The Kuiper Belt is a disk-like region from about 30 to 50 astronomical units beyond Neptune, made of icy bodies largely retained in situ after planet formation. The Oort Cloud is a spherical shell reaching thousands to a hundred thousand astronomical units, thought to be a comet reservoir formed when outer Solar System bodies were gravitationally scattered to distant orbits by the giant planets, so one is a flat disk nearby and the other a far spherical shell of different origin.
难度 专业 · 适合 高中(15-18) CC BY 4.0 · 已核验 · Verified 2026-08-23 · 2 条独立证据
来源 · Source

苏宜,《天文学新概论》第5版,科学出版社

Su Yi, Introduction to Astronomy, 5th ed., Science Press

#柯伊伯带 #奥尔特云 #彗星

行星的「核—幔分异」过程与磁场生成之间存在什么物理联系?

What physical link exists between a planet's core-mantle differentiation and the generation of its magnetic field?

核—幔分异指行星早期熔融时致密铁镍下沉形成金属核心、轻物质上浮成地幔的过程,释放的引力能使内部长期保持高温液态外核。液态金属外核的对流与行星自转耦合,通过发电机效应产生全球磁场,因此是否有活跃磁场往往取决于是否发生过充分分异并保有液态外核。
Core-mantle differentiation is the early molten-stage sinking of dense iron-nickel to form a metallic core and rising of lighter material into a mantle, and the released gravitational energy keeps the interior hot enough for a long-lived liquid outer core. Convection in that liquid metallic outer core, coupled with planetary rotation, generates a global magnetic field through the dynamo effect, so an active field usually depends on thorough differentiation and a retained liquid outer core.
难度 专业 · 适合 高中(15-18) CC BY 4.0 · 来源待核验 · Source pending review
来源 · Source

出处备注:著录仅给书名,无版次与年份;同一书名常对应多个版次,不臆测具体版本。

《天体物理学报》

Acta Astrophysica Sinica

#核幔分异 #发电机效应 #行星磁场

天王星大气与内部热力学有哪些尚未解释清楚的特征?

What poorly explained features remain in Uranus's atmosphere and internal thermodynamics?

天王星向外辐射的能量几乎等于吸收的阳光,内部热源异常微弱,与其姊妹星海王星形成鲜明对比,原因仍不明。其大气甲烷吸收导致极低的层顶温度,而甲烷与氢的混合物在深部高压下相态与对流模式也未被直接探测,使内部能量平衡成为未解问题。
Uranus radiates almost exactly as much energy as it absorbs from sunlight, with an anomalously weak internal heat source that contrasts sharply with Neptune, and the reason is unknown. Its methane absorption produces an extremely low tropopause temperature, while the phase behavior and convection of methane-hydrogen mixtures under deep high pressure remain unprobed, leaving its internal energy balance unsolved.
难度 专业 · 适合 高中(15-18) CC BY 4.0 · 来源待核验 · Source pending review
来源 · Source

出处备注:本题原挂出处与答案内容不符,已撤回;具体书目待补,暂不展示来源。

本题原挂出处与答案内容不符,已撤回;具体书目待补。

Previous citation withdrawn as unsupported for this answer; a specific source is pending.

#天王星 #内部热源 #甲烷大气

木卫二(Europa)为何被认为具备潜在宜居环境?

Why is Jupiter's moon Europa considered to have a potentially habitable environment?

木卫二表面覆盖冰壳,其下被潮汐加热维持着全球性的液态咸水海洋,体积可能超过地球海水总和。冰下海洋与岩石海床接触可提供能量与矿物质,而欧罗巴快船等任务正调查其冰壳厚度与喷流,评估生命存在的可能。
Europa is sheathed in an ice shell beneath which tidal heating sustains a global salty liquid ocean that may hold more water than all Earth's oceans. The ocean's contact with a rocky seafloor can supply energy and minerals, and missions such as Europa Clipper are investigating ice thickness and plumes to assess the prospect of life.
难度 进阶 · 适合 初中(12-15) CC BY 4.0 · 已核验 · Verified 2026-08-23 · 2 条独立证据
来源 · Source

苏宜,《天文学新概论》第5版,科学出版社

Su Yi, Introduction to Astronomy, 5th ed., Science Press

#木卫二 #冰下海洋 #潮汐加热

太阳系中的「冰巨星」指哪两颗行星,有什么特点?

Which two planets are the ice giants of the Solar System, and what are their traits?

冰巨星指天王星与海王星,与以氢氦为主的气态巨行星不同,它们主要由水、氨、甲烷等「冰」物质与岩石核心构成。它们体积小于木星土星,但拥有浓密甲烷大气而呈蓝绿色,且天王星以近直角「躺着」自转,磁场也明显偏离中心。
The ice giants are Uranus and Neptune; unlike the hydrogen-helium gas giants, they are built mainly from ices such as water, ammonia, and methane atop rocky cores. Smaller than Jupiter and Saturn, they have dense methane atmospheres giving a blue-green hue, and Uranus rotates nearly on its side while possessing a markedly off-center magnetic field.
难度 进阶 · 适合 大众 CC BY 4.0 · 已核验 · Verified 2026-08-23 · 2 条独立证据
来源 · Source

苏宜,《天文学新概论》第5版,科学出版社

Su Yi, Introduction to Astronomy, 5th ed., Science Press

#冰巨星 #天王星 #海王星

从资源角度看,小行星采矿主要瞄准哪些类型的天体?

From a resource perspective, which types of bodies does asteroid mining mainly target?

小行星采矿通常瞄准近地小行星中的 M 型(金属型)天体,富含铁、镍与铂族金属,以及 C 型(碳质)天体,可能携带水冰与有机化合物。前者可用于空间制造与稀有金属,后者既能提供推进剂用的水,也可能含生命相关前体物质。
Asteroid mining typically targets M-type (metallic) near-Earth asteroids rich in iron, nickel, and platinum-group metals, and C-type (carbonaceous) bodies that may carry water ice and organics. The former serve space manufacturing and rare metals, while the latter can supply water for propellant and possibly prebiotic material.
难度 进阶 · 适合 初中(12-15) CC BY 4.0 · 已核验 · Verified 2026-08-23 · 2 条独立证据
来源 · Source

苏宜,《天文学新概论》第5版,科学出版社

Su Yi, Introduction to Astronomy, 5th ed., Science Press

#小行星采矿 #M型小行星 #C型小行星

太阳系中的「特洛伊小行星」分布在什么地方?

Where are the Trojan asteroids of the Solar System located?

特洛伊小行星聚集在行星轨道上的拉格朗日点 L4 与 L5 附近,与行星同步绕太阳运行而长期保持稳定。最著名的是木星特洛伊群,数量以十万计;2021 年露西号任务正是赴外太阳系探访这些早期太阳系的「化石」。
Trojan asteroids cluster near the L4 and L5 Lagrange points of a planet's orbit, co-orbiting the Sun with the planet in long-term stable configurations. The best known are the Jupiter Trojans, numbering in the hundreds of thousands; NASA's 2021 Lucy mission was launched to visit these fossils of the early Solar System.
难度 进阶 · 适合 大众 CC BY 4.0 · 已核验 · Verified 2026-08-23 · 2 条独立证据
来源 · Source

苏宜,《天文学新概论》第5版,科学出版社

Su Yi, Introduction to Astronomy, 5th ed., Science Press

#特洛伊小行星 #拉格朗日点 #露西号

国际天文学联合会是如何定义「矮行星」的?

How does the International Astronomical Union define a dwarf planet?

根据 2006 年 IAU 决议,矮行星是围绕太阳运行、自身引力足以呈近球形、但尚未清空轨道附近其他天体的天体。冥王星、谷神星、阋神星均属此类,因未清空轨道邻近区域而被排除出行星行列。
Per the 2006 IAU resolution, a dwarf planet orbits the Sun, is massive enough for a near-spherical shape under its own gravity, but has not cleared its orbital neighborhood of other bodies. Pluto, Ceres, and Eris fall in this class and were excluded from full planet status because they failed to clear their neighborhoods.
难度 进阶 · 适合 初中(12-15) CC BY 4.0 · 已核验 · Verified 2026-08-23 · 2 条独立证据
来源 · Source

苏宜,《天文学新概论》第5版,科学出版社

Su Yi, Introduction to Astronomy, 5th ed., Science Press

#矮行星 #冥王星 #IAU定义