Jove
Visualize
联系我们
JoVE
x logofacebook logolinkedin logoyoutube logo
关于 JoVE
概览领导团队博客JoVE 帮助中心
作者
出版流程编辑委员会范围与政策同行评审常见问题投稿
图书馆员
用户评价订阅访问资源图书馆顾问委员会常见问题
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experiments存档
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教师资源中心教师网站
使用条款与条件
隐私政策
政策

相关概念视频

Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Effects of EDTA on End-Point Detection Methods01:18

Effects of EDTA on End-Point Detection Methods

Different methods, such as visual observance of metal-ion indicators, spectroscopic techniques, and potentiometric methods, can determine the endpoint of an EDTA titration.
In the visual method, metal-ion indicators (metallochromic dyes), which have distinct colors in their free and complex forms, are added to the mixture to signal the titration's end point. They form stable complexes with metal ions, but these complexes are weaker than the corresponding metal–EDTA complexes. As a result, EDTA...
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
Atomic Absorption Spectroscopy: Interference01:25

Atomic Absorption Spectroscopy: Interference

Interference leads to systematic error in atomic absorption (AA) measurements by enhancing or diminishing the analytical signal or the background. These interferences can be grouped into three main categories: spectral interference, chemical interference, and physical interference.
Spectral interference occurs when signals from other elements or molecules overlap with the analyte signal, falsely elevating or masking the analyte's absorbance. This interference can be corrected using Zeeman,...
Elastic Collisions: Case Study01:15

Elastic Collisions: Case Study

Elastic collision of a system demands conservation of both momentum and kinetic energy. To solve problems involving one-dimensional elastic collisions between two objects, the equations for conservation of momentum and conservation of internal kinetic energy can be used. For the two objects, the sum of momentum before the collision equals the total momentum after the collision. An elastic collision conserves internal kinetic energy, and so the sum of kinetic energies before the collision equals...
Doppler Effect - II01:05

Doppler Effect - II

The Doppler effect has several practical, real-world applications. For instance, meteorologists use Doppler radars to interpret weather events based on the Doppler effect. Typically, a transmitter emits radio waves at a specific frequency toward the sky from a weather station. The radio waves bounce off the clouds and precipitation and travel back to the weather station. The radio frequency of the waves reflected back to the station appears to decrease if the clouds or precipitation are moving...

您也可能阅读

相关文章

通过共同作者、期刊和引用图与本文相关的文章。

排序
Same author

The Lucy flyby of (52246) Donaldjohanson: A bilobed asteroid with tumbling rotation.

Science (New York, N.Y.)·2026
Same author

A temperate Earth-sized planet with tidal heating transiting an M6 star.

Nature·2023
Same author

Orbital period change of Dimorphos due to the DART kinetic impact.

Nature·2023
Same author

Successful kinetic impact into an asteroid for planetary defence.

Nature·2023
Same author

Ejecta from the DART-produced active asteroid Dimorphos.

Nature·2023
Same author

The rotation of low mass stars at 30 Myr in the cluster NGC 3766.

Proceedings of the International Astronomical Union. International Astronomical Union·2020

相关实验视频

Updated: Jul 16, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

对小行星YORP效应的直接检测.

Stephen C Lowry1, Alan Fitzsimmons, Petr Pravec

  • 1School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK. s.c.lowry@qub.ac.uk

Science (New York, N.Y.)
|March 10, 2007
PubMed
概括

雅尔科夫斯基-奥基夫-拉德泽夫斯基-帕达克 (YORP) 效应提供了改变小行星旋转速率的直接证据. 对近地小行星2000 PH5的精确观测显示其旋转的持续增加,证实了YORP效应.

更多相关视频

Measuring the Behavioral Effects of Intraocular Scatter
05:10

Measuring the Behavioral Effects of Intraocular Scatter

Published on: February 18, 2021

Detection and Recovery of Palladium, Gold and Cobalt Metals from the Urban Mine Using Novel Sensors/Adsorbents Designated with Nanoscale Wagon-wheel-shaped Pores
10:31

Detection and Recovery of Palladium, Gold and Cobalt Metals from the Urban Mine Using Novel Sensors/Adsorbents Designated with Nanoscale Wagon-wheel-shaped Pores

Published on: December 6, 2015

相关实验视频

Last Updated: Jul 16, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Measuring the Behavioral Effects of Intraocular Scatter
05:10

Measuring the Behavioral Effects of Intraocular Scatter

Published on: February 18, 2021

Detection and Recovery of Palladium, Gold and Cobalt Metals from the Urban Mine Using Novel Sensors/Adsorbents Designated with Nanoscale Wagon-wheel-shaped Pores
10:31

Detection and Recovery of Palladium, Gold and Cobalt Metals from the Urban Mine Using Novel Sensors/Adsorbents Designated with Nanoscale Wagon-wheel-shaped Pores

Published on: December 6, 2015

科学领域:

  • 太阳系动力学 太阳系动力学
  • 小行星物理学 小行星物理学
  • 观测天文学 观测天文学

背景情况:

  • 雅尔科夫斯基-奥基夫-拉德泽夫斯基-帕达克效应 (YORP) 是一种理论上的机制,影响太阳系中小型天体的旋转.
  • 以前对YORP效应的证据是间接的,缺乏确定的观察证据.

研究的目的:

  • 提供对YORP效应对小行星旋转状态的影响的直接观测证据.
  • 精确测量一个小近地小行星的自转速率变化.

主要方法:

  • 在4年的时间里对小行星 (54509) 2000 PH5进行了精确的光学摄影测量观测.
  • 分析了观测数据,以确定小行星的旋转速度及其随时间的变化.
  • 进行了动态模拟,包括引力扭矩分析和近地方法建模,以排除其他解释.

主要成果:

  • 观测到小行星2000 PH5.5的旋转速度不断增加.
  • 将旋转速率的增加量化为domega/dt=2.0 (+/-0.2) x 10(-4) 度每天平方.
  • 证明来自地球碰撞的引力扭矩无法解释观测到的旋转加速.

结论:

  • 在小行星2000 PH5中观察到的旋转速度增加为YORP效应提供了直接证据.
  • 动态模拟支持YORP效应作为旋转变化的原因.
  • 预计小行星2000 PH5在未来可能达到大约20秒的旋转周期.