相关实验视频
Updated: Mar 30, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
11.1K
围绕火星的轨道高度的尘埃观测
L Andersson1, T D Weber2, D Malaspina2
1Laboratory for Atmospheric and Space Physics, University of Colorado-Boulder, Boulder, CO 80303, USA. laila.andersson@lasp.colorado.edu.
概括
已经观察到行星间的尘埃颗粒进入火星的大气层. 这一发现挑战了关于尘埃运输的先前假设,
科学领域:
- 星球科学
- 大气科学
- 天文地质学
背景情况:
- 尘埃在火星表面附近普遍存在,但其在高海拔 (>150公里) 的存在是已知的大气过程无法解释的.
- 之前的模型没有考虑到火星上150公里以上高度的尘埃度.
研究的目的:
- 在火星大气层的高海拔地区调查尘埃的存在和起源.
- 分析观测到的尘埃粒子的特性及其对行星间尘埃动态的影响.
主要方法:
- 在火星大气和挥发性进化 (MAVEN) 飞船上使用了朗穆尔探测器和波浪仪器.
- 分析了从150公里到1000公里以上的尘埃分布数据.
- 将观测数据与实验室测量尘埃特性进行比较.
主要成果:
- 检测到的尘埃高度远远高于之前所认为的,从150公里到1000公里以上.
- 解释观察到的尘埃分布为星际起源的迹象.
- 估计粉尘粒大小在1至12微米之间,假设速度为~18公里/秒.
结论:
- 证实了行星间尘埃进入火星大气层的存在.
- 提供了直接的证据,改善了对行星间尘埃来源,沉和太阳系内部的传输的理解.
- 突出了这种尘埃对火星大气过程的影响.
相关概念视频
Kepler's First Law of Planetary Motion
6.1K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
6.1K
Acceleration due to Gravity on Other Planets
5.2K
The gravitational acceleration of an object near the Earth's surface is called the acceleration due to gravity. It can be measured by conducting simple experiments on Earth. However, such an experiment is impossible to conduct on the surface of other planets.
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
5.2K
Flame Photometry: Lab
1.2K
In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...
1.2K
Torque Free Motion
909
The torque-free motion refers to the movement of a rigid body in space when no external torques are acting upon it. This type of motion can be observed in environments where there are no external forces or frictions, like in outer space. For example, a rotation of Mars in space is a torque-free motion. Mars is an axisymmetric object, meaning it has an axis of symmetry along which it rotates, designated as the z-axis. The rotating frame of reference is defined such that the center of mass of...
909
Circular Orbits and Critical Velocity for Satellites
5.7K
The Moon orbits around the Earth. In turn, the Earth (and other planets) orbit the Sun. The space directly above our atmosphere is filled with artificial satellites in orbit. One can examine the circular orbit, the simplest kind of orbit, to understand the relationship between the speed and the period of planets and satellites with respect to their positions and the bodies that they orbit.
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
5.7K
Flame Photometry: Overview
1.9K
Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
1.9K

