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

Kinetic Molecular Theory and Gas Laws Explain Properties of Gas Molecules02:34

Kinetic Molecular Theory and Gas Laws Explain Properties of Gas Molecules

30.4K
The test of the kinetic molecular theory (KMT) and its postulates is its ability to explain and describe the behavior of a gas. The various gas laws (Boyle’s, Charles’s, Gay-Lussac’s, Avogadro’s, and Dalton’s laws) can be derived from the assumptions of the KMT, which have led chemists to believe that the assumptions of the theory accurately represent the properties of gas molecules.
30.4K
Behavior of Gas Molecules: Molecular Diffusion, Mean Free Path, and Effusion03:48

Behavior of Gas Molecules: Molecular Diffusion, Mean Free Path, and Effusion

24.5K
Although gaseous molecules travel at tremendous speeds (hundreds of meters per second), they collide with other gaseous molecules and travel in many different directions before reaching the desired target. At room temperature, a gaseous molecule will experience billions of collisions per second. The mean free path is the average distance a molecule travels between collisions. The mean free path increases with decreasing pressure; in general, the mean free path for a gaseous molecule will be...
24.5K
Nuclear Fusion02:45

Nuclear Fusion

33.2K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
33.2K
Detection of Black Holes01:10

Detection of Black Holes

1.7K
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...
1.7K
Escape Velocities of Gases01:19

Escape Velocities of Gases

1.6K
To escape the Earth's gravity, an object near the top of the atmosphere at an altitude of 100 km must travel away from Earth at 11.1 km/s. This speed is called the escape velocity. The temperature at which gas molecules attain the rms speed, which is equal to the escape velocity, can be estimated by using the equation for the average kinetic energy of the gas molecules. According to the kinetic theory of gas, the average kinetic energy of the gas molecules is proportional to its...
1.6K
Gas Solubility01:31

Gas Solubility

136
Gas solubility in liquids forms liquid-gas solutions, such as soft drinks, where carbon dioxide is dissolved in water, and the ocean, where the solubility of oxygen and carbon dioxide supports marine life. The ability of oceans to dissolve gases impacts weather conditions in the troposphere.However, gas-liquid interactions vary. For instance, hydrogen chloride gas is highly soluble in water, while oxygen's solubility is much lower. Because these solutions are non-ideal, Raoult’s law,...
136

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

Resolved ALMA observations of water in the inner astronomical units of the HL Tau disk.

Nature astronomy·2024
Same author

Streamers feeding the SVS13-A protobinary system: astrochemistry reveals accretion shocks?

Faraday discussions·2023
Same author

Exploring the link between star and planet formation with Ariel.

Experimental astronomy·2022
Same author

Reflective Toraldo pupil for high-resolution millimeter-wave astronomy.

Applied optics·2020
Same author

Toward the RNA-World in the Interstellar Medium-Detection of Urea and Search of 2-Amino-oxazole and Simple Sugars.

Astrobiology·2020
Same author

Design of discrete and continuous super-resolving Toraldo pupils in the microwave range.

Applied optics·2018

相关实验视频

Updated: May 5, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

15.6K

作为恒星形成机制的气体流入,恒星的质量高达太阳的20倍.

Maria T Beltrán1, Riccardo Cesaroni, Claudio Codella

  • 1Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal, 647, 08028, Barcelona, Catalunya, Spain. mbeltran@am.ub.es

Nature
|September 29, 2006
PubMed
概括

大质量恒星通过非球形积累形成,尽管有强烈的辐射,但允许气体流入. 观测证实了这一过程,显示气体落在一个年轻,巨大的恒星上.

科学领域:

  • 天文学 天文学
  • 天体物理学 天体物理学
  • 恒星进化 恒星进化

背景情况:

  • 低质量恒星通过增加气体而生长,这种过程在巨大的恒星 (>10太阳质量) 中受到强烈辐射的限制.
  • 恒星的存在>10太阳质量表明替代形成机制是必要的.
  • 非球形积累,即辐射沿轴逃逸,是大质量恒星形成的一个解决方案.

研究的目的:

  • 为了研究高质量恒星的形成机制.
  • 为了测试非球形积累促进超过8太阳质量的恒星形成的假设.
  • 为在非常年轻的大质量恒星上增加气体提供观测证据.

主要方法:

  • 在一个高质量恒星形成区域观察到氨线排放.
  • 分析了氨线,以推断气体运动和积累.
  • 专注于一个特定的年轻,巨大的恒星候选者 (大约20个太阳质量).

主要成果:

  • 检测到气体向一个非常年轻的恒星移动.
  • 观测到的增长速度与大约20个太阳质量的恒星一致.
  • 这些发现支持了高质量恒星形成的非球形积累理论.

更多相关视频

Formation of Thick Dense Yttrium Iron Garnet Films Using Aerosol Deposition
10:52

Formation of Thick Dense Yttrium Iron Garnet Films Using Aerosol Deposition

Published on: May 15, 2015

9.0K
Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer
07:24

Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer

Published on: February 19, 2018

8.8K

相关实验视频

Last Updated: May 5, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

15.6K
Formation of Thick Dense Yttrium Iron Garnet Films Using Aerosol Deposition
10:52

Formation of Thick Dense Yttrium Iron Garnet Films Using Aerosol Deposition

Published on: May 15, 2015

9.0K
Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer
07:24

Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer

Published on: February 19, 2018

8.8K

结论:

  • 非球形积累为超过10太阳质量的恒星形成提供了可行的途径.
  • 观察到的氨线证实了气体流入到一个年轻的大恒星上,与理论模型保持一致.
  • 这项研究提供了关键的观测证据,说明宇宙中最大质量的恒星是如何诞生的.