Vật lý thiên văn

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Vật lý thiên văn là một phần của ngành thiên văn học có quan hệ với vật lý trong vũ trụ, bao gồm các tính chất vật lý (cường độ ánh sáng, tỉ trọng, nhiệt độ, và các thành phần hóa học) của các thiên thể chẳng hạn như ngôi sao, thiên hà, và interstellar medium, cũng như các ảnh hưởng qua lại của chúng. Công việc nghiên cứu Vật lý vũ trụ học là vật lý thiên văn mang tính lý thuyết trong phạm vi rộng nhất.

Bởi vì ngành vật lý thiên văn là một lĩnh vực mênh mông , nên các nhà vật lý học thiên thể thường áp dụng các ngành khoa học khác trong vật lý, bao gồm cơ khí, điện từ học, cơ học thống kê, nhiệt động lực học, cơ học lượng tử, tính tương đối, vật lý nguyên tử, vật lý hạt nhân, và vật lý nguyên tử, phân tử và quang học. Trong thực nghiệm, ngành nghiên cứu thiên văn hiện đại bao gồm một phần quan trọng dựa trên nền tảng vật lý cơ bản. Tên gọi của ngành học trong các trường đại học ("vật lý thiên văn" hay "thiên văn học") thường liên quan nhiều đến lịch sử của ngành hơn là nội dung nghiên cứu. Vật lý thiên văn được đào tạo trong rất nhiều trường đại học với bằng cử nhân, thạc sĩ, tiến sĩ thông qua các khoa như kỹ thuật hàng không vũ trụ, vật lý hoặc thiên văn học.

Mục lục 1 Lịch sử 2 Đối tượng của ngành vật lý thiên văn 3 Theoretical astrophysics 4 See also 5 Tham khảo 6 Các liên kết ngoài

[sửa] Lịch sử

Mặc dù thiên văn học đã có lịch sử lâu đời nhưng vẫn được xét là một ngành riêng biệt với vật lý. Trong quan điểm về thế giới của Aristotle, the celestial pertained to perfection—bodies in the sky being perfect spheres moving in perfectly circular orbits—while the earthly pertained to imperfection; these two realms were not seen as related.

Aristarchus of Samos (c.310-c.250 BC) first put forward that the motions of the celestial bodies could be explained by assuming that the Earth and all the other planets in the Solar System orbited the Sun. Aristarchus' heliocentric theory was not accepted in the Ancient Greek world and for centuries, the apparently common-sense view that the Sun and other planets went round the Earth went basically unquestioned, until Nicolaus Copernicus revived the heliocentric model in the 16th century. In 1609, Galileo Galilei discovered the four brightest moons of Jupiter, and documented their orbits about that planet, which contradicted the geocentric dogma of the Catholic Church of his time, and escaped serious punishment only by maintaining that his astronomy was a work of mathematics, not of natural philosophy (physics), and therefore purely abstract.

The availability of accurate observational data mainly from the observatory of Tycho Brahe led to research into theoretical explanations for the observed behavior. At first, only empirical rules were discovered, such as Kepler's laws of planetary motion, discovered at the start of the 17th century. Later that century, Isaac Newton bridged the gap between Kepler's laws and Galileo's dynamics, discovering that the same laws that rule the dynamics of objects on earth rule the motion of planets and the moon. Celestial mechanics, the application of Newtonian gravity and Newton's laws to explain Kepler's laws of planetary motion, was the first unification of astronomy and physics.

After Isaac Newton published his Principia, maritime navigation was transformed. Starting around 1670, the entire world was measured using essentially modern latitude instruments and the best available clocks. The needs of navigation provided a drive for progressively more accurate astronomical observations and instruments, providing a background for ever more available data for scientists.

At the end of the 19th century, it was discovered that, when decomposing the light from the Sun, a multitude of spectral lines were observed (regions where there was less or no light). Experiments with hot gases showed that the same lines could be observed in the spectra of gases, specific lines corresponding to unique chemical elements. In this way it was proved that the chemical elements found in the Sun(chiefly hydrogen) were also found on Earth. Indeed, the element helium was first discovered in the spectrum of the sun and only later on earth, hence its name. During the 20th century, spectroscopy (the study of these spectral lines) advanced, particularly as a result of the advent of quantum physics that was necessary to understand the astronomical and experimental observations.^[1]

See also:

• Timeline of knowledge about galaxies, clusters of galaxies, and large-scale structure
• Timeline of white dwarfs, neutron stars, and supernovae
• Timeline of black hole physics
• Timeline of gravitational physics and relativity

[sửa] Đối tượng của ngành vật lý thiên văn

Most astrophysical processes cannot be reproduced in laboratories on Earth. However, there is a huge variety of astronomical objects visible all over the electromagnetic spectrum. The study of these objects through passive collection of data is the goal of observational astrophysics.

The equipment and techniques required to study an astrophysical phenomenon can vary widely. Many astrophysical phenomena that are of current interest can only be studied by using very advanced technology and were simply not known until very recently.

The majority of astrophysical observations are made using the electromagnetic spectrum.

• Radio astronomy studies radiation with a wavelength greater than a few millimeters. Radio waves are usually emitted by cold objects, including interstellar gas and dust clouds. The cosmic microwave background radiation is the redshifted light from the Big Bang. Pulsars were first detected at microwave frequencies. The study of these waves requires very large radio telescopes.
• Infrared astronomy studies radiation with a wavelength that is too long to be visible but shorter than radio waves. Infrared observations are usually made with telescopes similar to the usual optical telescopes. Objects colder than stars (such as planets) are normally studied at infrared frequencies.
• Optical astronomy is the oldest kind of astronomy. Telescopes paired with a charge-coupled device or a spectroscope are the most common instruments used. The Earth's atmosphere interferes somewhat with optical observations, so adaptive optics and space telescopes are used to obtain the highest possible image quality. In this range, stars are highly visible, and many chemical spectra can be observed to study the chemical composition of stars, galaxies and nebulae.
• Ultraviolet, X-ray and gamma ray astronomy study very energetic processes such as binary pulsars, black holes, magnetars, and many others. These kinds of radiation do not penetrate the Earth's atmosphere well, so they are studied with space-based telescopes such as RXTE, the Chandra X-ray Observatory and the Compton Gamma Ray Observatory.

Other than electromagnetic radiation, few things may be observed from the Earth that originate from great distances. A few gravitational wave observatories have been constructed, but gravitational waves are extremely difficult to detect. Neutrino observatories have also been built, primarily to study our Sun. Cosmic rays consisting of very high energy particles can be observed hitting the Earth's atmosphere.

Observations can also vary in their time scale. Most optical observations take minutes to hours, so phenomena that change faster than this cannot readily be observed. However, historical data on some objects is available spanning centuries or millennia. On the other hand, radio observations may look at events on a millisecond timescale (millisecond pulsars) or combine years of data (pulsar deceleration studies). The information obtained from these different timescales is very different.

The study of our own Sun has a special place in observational astrophysics. Due to the tremendous distance of all other stars, the Sun can be observed in a kind of detail unparalleled by any other star. Our understanding of our own sun serves as a guide to our understanding of other stars.

The topic of how stars change, or stellar evolution, is often modelled by placing the varieties of star types in their respective positions on the Hertzsprung-Russell diagram, which can be viewed as representing the state of a stellar object, from birth to destruction. The material composition of the astronomical objects can often be examined using:

• Spectroscopy
• Radio astronomy
• Neutrino astronomy (future prospects)

[sửa] Theoretical astrophysics

Theoretical astrophysics is the discipline that seeks to explain the phenomena observed by astronomers in physical terms with a theoretic approach. With this purpose, theoretical astrophysicists create and evaluate models and physical theories to reproduce and predict the observations. In most cases, trying to figure out the implications of physical models is not easy and takes a lot of time and effort.

Theoretical astrophysicists use a wide variety of tools which include analytical models (for example, polytropes to approximate the behaviors of a star) and computational numerical simulations. Each has some advantages. Analytical models of a process are generally better for giving insight into the heart of what is going on. Numerical models can reveal the existence of phenomena and effects that would otherwise not be seen.^[2][3]

Theorists in astrophysics endeavor to create theoretical models and figure out the observational consequences of those models. This helps allow observers to look for data that can refute a model or help in choosing between several alternate or conflicting models.

Theorists also try to generate or modify models to take into account new data. In the case of an inconsistency, the general tendency is to try to make minimal modifications to the model to fit the data. In some cases, a large amount of inconsistent data over time may lead to total abandonment of a model.

Within the astronomical community, theorists are widely caricatured as being mechanically inept and unlucky for observational efforts. Having a theorist at an observatory is considered likely to jinx an observation run and cause machines to break inexplicably or to have the sky cloud over.

Topics studied by theoretical astrophysicists include: stellar dynamics and evolution; galaxy formation; large-scale structure of matter in the Universe; origin of cosmic rays; general relativity and physical cosmology, including string cosmology and astroparticle physics. Astrophysical relativity serves as a tool to gauge the properties of large scale structures for which gravitation plays a significant role in physical phenomena investigated and serves as the basis for black hole (astro)physics and the study of gravitational waves.

Some widely-accepted and studied theories and models in astrophysics, now included in the Lambda-CDM model are the Big Bang, Cosmic inflation, dark matter, and fundamental theories of physics.

A few examples of this process:

Physical process	Experimental tool	Theoretical model	Explains/predicts
Gravitation	Radio telescopes	Self-gravitating system	Emergence of a star system
Nuclear fusion	Spectroscopy	Stellar evolution	How the stars shine and how metals formed
The Big Bang	Hubble Space Telescope, COBE	Expanding universe	Age of the Universe
Quantum fluctuations		Cosmic inflation	Flatness problem
Gravitational collapse	X-ray astronomy	General relativity	Black holes at the center of Andromeda galaxy
CNO cycle in stars

Dark matter and dark energy are the current leading topics in astrophysics, as their discovery and controversy originated during the study of the galaxies.

[sửa] See also

• Astronomical observatories
• Important publications in astrophysics
• List of astrophysicists
• Nucleosynthesis
• Particle accelerator
• Astrodynamics

[sửa] Tham khảo

[sửa] Các liên kết ngoài

• Prof. Sir Harry Kroto, NL, Astrophysical Chemistry Lecture Series. 8 Freeview Lectures provided by the Vega Science Trust.
• 'The Mathematician Who Can't Add Up' Cosmologist Emma King Freeview 'Snapshots video' by the Vega Science Trust.
• Stanford Linear Accelerator Center, Stanford, California
• Search for astrophysics
• overinflation.org Astrophysics and Cosmology News