相关实验视频
Updated: Apr 1, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
20.3K
在AU显微镜周围的碎片盘中快速移动的特征
Anthony Boccaletti1, Christian Thalmann2, Anne-Marie Lagrange3,4
1LESIA, Observatoire de Paris, CNRS, Université Paris Diderot, Université Pierre et Marie Curie, 5 place Jules Janssen, 92190 Meudon, France.
Nature
|October 10, 2015
概括
天文学家在AU Microscopii碎片盘中观察到一些不寻常的特征. 这些动态结构远离恒星挑战了当前的行星形成理论.
科学领域:
- 天文学与天体物理学
- 外行星科学
背景情况:
- 围绕主序恒星运行的碎片盘是红外辐射的来源,最初被认为是行星形成的副产品.
- 碎片盘中的不对称性,比如Pictoris系统中的不对称性,与行星的引力扰动有关.
- AU Microscopii碎片盘以其边缘方向和局部强度变化而闻名,为研究磁盘动态提供了一个独特的案例.
研究的目的:
- 在AU Microscopii碎片盘中调查之前观察到的不对称结构的性质和起源.
- 通过高对比度成像来描述这些特征的形态,定位和时间演变.
主要方法:
- 使用高对比度成像技术观察AU微镜碎片盘.
- 在几年内分析图像以识别和跟踪磁盘中的大规模特征.
主要成果:
- 在 AU 显微镜盘的东南侧发现了一系列五个大尺度的特征, 跨越10-60天文单位.
- 观察到这些特征持续1-4年,并以预计的4-10公里/秒的速度远离恒星.
- 观察到的特征表现出快速的进化,挑战现有的模型.
结论:
- 这些特征的起源,定位,形态和快速向外运动很难用当前的行星形成和盘进化理论来解释.
- 这些发现表明AU Microscopii碎片盘中存在需要进一步调查的动态过程或实体.
- 这项研究突显了碎片盘的复杂性以及超越标准行星系统形成模型发现新现象的潜力.
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
Phase Contrast and Differential Interference Contrast Microscopy
15.2K
Phase-Contrast Microscopes
In-phase-contrast microscopes, interference between light directly passing through a cell and light refracted by cellular components is used to create high-contrast, high-resolution images without staining. It is the oldest and simplest type of microscope that creates an image by altering the wavelengths of light rays passing through the specimen. Altered wavelength paths are created using an annular stop in the condenser. The annular stop produces a hollow cone of...
In-phase-contrast microscopes, interference between light directly passing through a cell and light refracted by cellular components is used to create high-contrast, high-resolution images without staining. It is the oldest and simplest type of microscope that creates an image by altering the wavelengths of light rays passing through the specimen. Altered wavelength paths are created using an annular stop in the condenser. The annular stop produces a hollow cone of...
15.2K
Atomic Force Microscopy
4.7K
Atomic force microscopy (AFM) is a type of scanning probe microscopy that can analyze topographic details of various specimens like ceramics, glass, polymers, and biological samples. AFM offers over 1000 times more resolution than the optical imaging system. Images generated from AFM are three-dimensional surface profiles, offering an advantage over the flat, two-dimensional images from other imaging techniques.
The AFM Probe
The probe is regarded as the heart of any AFM setup and comprises the...
The AFM Probe
The probe is regarded as the heart of any AFM setup and comprises the...
4.7K
Atomic Emission Spectroscopy: Overview
4.3K
Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
4.3K
Detection of Black Holes
2.6K
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...
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...
2.6K
Scanning Electron Microscopy
6.0K
A scanning electron microscope (SEM) is used to study the surface features of a sample by using an electron beam that scans the sample surface in a two-dimensional manner. Typically, areas between ~1 centimeter to 5 micrometers in width can be imaged. SEM can be used to image bacteria, viruses, tissues as well as larger samples like insects. Conventional SEM gives a magnification ranging from 20X to 30,000X and spatial resolution of 50 to 100 nanometers.
Fundamental Principles
Accelerated...
Fundamental Principles
Accelerated...
6.0K

