Astrophysics

Subject name
open 2 entries with the same name
Collection
zero Useful+1
zero
Astrophysics is not only a major branch of astronomy, but also one of the branches of physics. It is a discipline that uses the technology, methods and theories of physics to study the shape, structure, physical conditions, chemical composition and evolution laws of celestial bodies.
Analysis of astrophysical electromagnetic radiation Various physical parameters of celestial bodies can be obtained. According to these parameters, the physical theory is used to clarify the physical process , and its evolution is Measured astrophysics And theoretical astrophysics.
Some strange phenomena found on celestial bodies can also inspire and promote Modern Physics The extreme conditions and Cosmic environment It provides an excellent natural laboratory for physics.
and Theoretical physics Radiation in Nucleus , gravity Plasma , solid and Elementary particle For research a quasar cosmic ray , black hole Pulsar Interstellar dust Supernova explosion Laid the foundation.
Chinese name
Astrophysics
Foreign name
Astrophysics
Research object
universe
Category
Solar physics, galaxy astronomy, etc
Academic field
Mechanics, relativity, particle physics, etc
Characters
Einstein Hubble etc.
Discipline code
sixteen thousand and twenty [1-2]

development

Announce
edit
Astrophysics
From 129 BC ancient Greek astronomer Hipachas Visual inspection fixed star From the luminosity, Galileo used it in 1609 Optical telescope Observing celestial bodies, drawing Lunar chart , discovered by Huygens in 1655 – 1656 Saturn's rings And the Orion Nebula. Later, Harley discovered the stellar self, which was created by Herschel in the 18th century Stellar astronomy This is the gestation period of astrophysics.
In the middle of the 19th century, there were three Physical methods ——Spectroscopy Photometry and Photography Widely used in celestial bodies Observational research Later, the research on the structure, chemical composition and physical state of celestial bodies formed a complete scientific system, and astrophysics began to become an independent branch of astronomy.
The development of astrophysics has promoted Astronomical observation And research continue to produce new results and discoveries.
In 1859, Kirchhoff Solar spectrum Of Absorption line (i.e Fraunhofer spectral line )Make Scientific interpretation He thinks the absorption line is photosphere Issued Continuous spectrum Absorbed by the solar atmosphere, this discovery has promoted astronomers Spectroscope Study stars.
In 1864, Hagens Use height Dispersion Of Spectrograph Observing stars to identify the Spectral line , according to Doppler effect And measured some more Apparent velocity of star
In 1885, Pickering use first Object end prism Take spectrum Spectral classification By Planetary nebula and Diffuse nebula Research on Andromeda Nebula New stars are found in. These discoveries make astrophysics develop in breadth and depth.
In 1859, Kirchhoff according to thermodynamics Law interpretation Solar spectral Fraunhofer lines , asserting that there are some chemical element , which shows that you can use Theoretical physics This is the beginning of theoretical astrophysics.
The development of theoretical astrophysics is closely dependent on Theoretical physics Almost every important breakthrough in theoretical physics will greatly promote the progress of theoretical astrophysics.
In the early 1920s, Quantum Theory The establishment of, which makes it possible to analyze the spectrum of stars in depth Stellar atmosphere Of system theory
1930s Nuclear physics With the development of, the problem of stellar energy has been solved satisfactorily, and the theory of stellar internal structure has developed rapidly; And based on Herotu The measured results of Stellar evolution Of scientific theory
In 1917, Einstein used General relativity Analyzing the structure of the universe Relativistic cosmology
In 1920, Saha proposed stellar atmosphere Ionization theory Through the research of Emden, Schwarzenegger, Eddington and others Stellar interior The theory of structure has gradually matured.
In 1905, Herzpoon divided some stars into giant stars and dwarf star
In 1913, Russell Press Absolute magnitude Mapping stars with spectral patterns Distribution map , namely Herot chart.
In 1916, Adams and Kirscht found that there were slight differences between the spectra of giant stars and dwarf stars with the same spectral type, and established the spectral parallax method to calculate distance.
In 1938, Bette It is proposed that Thermonuclear reaction Theory, successfully solved Main sequence star Production capacity mechanism.
In 1929, Hubble was studying Extragalactic galaxy Spectrum, proposed Hubble's law , which greatly promoted Galactic astronomy Development of.
1931 – 1932, Jansky Found a Galactic center Universe of direction radio waves In the 1940s, Britain military radar Found sunlight Since then, radio astronomy has flourished; In the 1960s, it was discovered again by radio astronomy a quasar Pulsar Interstellar molecule , Microwave Background radiation
In 1946, the United States began shooting with rockets at an altitude of 30 – 100 kilometers above the ground Ultraviolet spectrum
In 1957, Soviet Union launch Artificial earth satellite , is the outer layer of the atmosphere Space observation Created conditions. Later, the United States Western Europe Japan has also successively launched Artificial satellite The world has launched a considerable number of Spacecraft , which is equipped with various types of detectors to detect the ultraviolet rays , X-ray Gamma ray Equal band radiation. Since then, astronomy has entered the era of full band observation.

definition

Announce
edit
Astrophysical diagram
Astrophysics is the physics of the universe, including the stars physical property (luminosity, density, temperature chemical composition And the interaction between stars and stars. Discussion on the Theory and Methods of Applied Physics Stellar structure Stellar evolution , the origin of the solar system cosmology Related issues.
Astrophysics involves a wide range of fields. Astrophysicists usually apply the methods of different disciplines, including mechanics electromagnetics statistical mechanics quantum mechanics relativity Particle physics And so on.
With the development of modern interdisciplinary science, it is closely related to chemistry, biology, history, computer, engineering, paleontology archaeology meteorology With a mixture of other disciplines, astrophysics has about 300 to 500 major professional branches, becoming the most cutting-edge leading discipline in physics, leading the major development of modern science and technology, and also the oldest Traditional science

research contents

Announce
edit

Test instrument

Astrophysics
Astrophysics experimental data Most rely on observation electromagnetic radiation get. Colder Astral body , like Interstellar matter or Interstellar cloud Will launch radio waves After the big explosion red shift The microwave left behind is called cosmic microwave Background radiation Studying these microwaves requires very large radio telescopes.
because Earth's atmosphere Interference, infrared ultraviolet rays Gamma ray and X-ray astronomy Must use Artificial satellite Make observation experiments outside the earth's atmosphere.
Optical astronomy Usually, additional installation is used Charge coupled element and a spectrometer To make observations. because atmosphere Will interfere observed data Must be equipped with an adaptive optical system, or Space telescope To get the best image. Here frequency domain Li, stellar visibility Very high. By observing the chemical spectrum, we can analyze fixed star Galaxy And the chemical composition of nebulae.
except cosmic ray Of Particle detection Meteoritic Laboratory analysis Spacecraft yes celestial bodies Field sampling and analysis, as well as the Gravitational wave In addition to observation, information about celestial bodies comes from electromagnetic radiation. The function of astrophysical instruments is to collect, locate, transform and analyze electromagnetic radiation. The collection and positioning of electromagnetic radiation are conducted by telescopes (including radio telescope )To achieve.
Radiative Continuous spectrum We can judge the mechanism of radiation and also know the surface temperature from Early type star Of Balmer system The surface pressure of the celestial body can be known from the jump above the limit; from UBV photometry system The luminosity and temperature values of stars can also be roughly determined. from Line spectrum More information can be obtained: Apparent velocity electron temperature electron density , chemical composition Excitation temperature End flow velocity. yes Konductra Of Observational research The radius, mass, luminosity and other important data of celestial bodies can be obtained. Research Pulsating variable star Of Photoperiod The relationship with luminosity can be determined Distance of celestial bodies

theoretical model

Theoretical celestial body physical scientist Tools for include analysis model and computer simulation The analytical model of astronomical process often enables scholars to have a deeper understanding of the internal mysteries; Computer simulation can show some very complex phenomena or effects.
Big Bang Model The two theoretical pillars of General relativity and Cosmological principle because Primordial nucleosynthesis The success of the theory and the cosmic microwave background radiation experiment confirmed that the scientists determined that the Big Bang model was correct. Scholars also created the Λ CDM model to explain the evolution of the universe, which covers Cosmic expansion (cosmic inflation)、 Dark energy dark substance And so on.
Radiation transfer theory It is a powerful tool to explain the known celestial phenomena, and can also predict the celestial bodies and celestial phenomena that have not yet been observed. Based on radiation transfer theory Stellar atmosphere theory , with heat nuclear fusion Concept based Element synthesis theory Theory of stellar internal structure and Celestial evolution theory , is Theoretical astrophysics The foundation of.

researcher

Astrophysics
Theoretical astrophysicists and measured astrophysicists respectively play the role of the two main researchers in this discipline, and the two have their own professional divisions. Theoretical astrophysicists usually play the role of bold hypothesis researchers. They constantly introduce new theories. They are less concerned about the verification of data. When the hypothesis is too high, it often evolves into Pseudoscience They are generally radical among astrophysical researchers.
Measured astrophysicists are usually proficient in theoretical astrophysics and, to a certain extent, have the ability to make their own Development theory , playing the role of a researcher who is careful to verify, usually physics positivism Believing only in observational data and often falsifying or confirming hypotheses proposed by theoretical astrophysics, practitioners of.

Research object

Announce
edit

solar system

The sun is the nearest ordinary star to the earth. The study of the sun has gone through the stages of studying its internal structure, energy source, chemical composition and static state surface structure , to use Multiband electromagnetic radiation The process of studying its activity phenomenon. solar wind The impact of Direct feeling The sun and the earth are closely related, so the study of earth science must take into account the sun's factors.
The study of planets is an important aspect of astrophysics.
In the past two decades, research on comets and Interplanetary matter Important achievements have been made in the research on the distribution, density, temperature, magnetic field and chemical composition of. along with Space exploration Progress, solar system And the research of the research of the research has become one of the most active fields.
For more than 200 years Origin and evolution of the solar system More than 40 theories have been put forward, but none of them is considered perfect and generally accepted.
In the past three decades, great progress has been made in this regard, and most astronomers agree that Stellar geochemistry It is the so-called "diffuse theory", but a few people believe that stars are transformed from super dense matter.

Special star

Special star More diverse: Cepheid variable The light change period of is 1~50 days, Light amplitude 0.1~2 the magnitude Long-period variable star The light variation period is 90~1000 days, and the light variation amplitude is 2.5~9 magnitudes; RR Lyrae variable The light variation period of is 0.05~1.5 days, and the light variation amplitude does not exceed 1~2 magnitudes; Taurus T-type variable star turns irregular light into various stars for research Formation and evolution of stars The rule provides samples. In addition, the special physical conditions on the celestial bodies are often not available on the earth. It is an important function of astrophysics to explore physical laws by using celestial phenomena.

Galaxy

Through years of research, people have Galaxy And the position of the sun in the Milky Way. The Milky Way is 100000 light years in diameter and 20000 light years thick. Through the study of the Milky Way fixed star The Group's research, establishment and validation Astral family and Galaxy Sub system And so on. yes Galaxy rotation Swivel arm Structure Silver nucleus and Silver halo A great deal of research has also been carried out.
Extragalactic galaxy It belongs to the same celestial level as the Milky Way. Galaxies can be roughly divided into five categories according to their shapes: Spiral galaxy Barred spiral galaxy , lenticular galaxy Elliptical galaxy Irregular galaxy Press Mass of galaxies Size can also be divided into Dwarf galaxy Giant galaxy Supergiant galaxy Their mass is about one million to one billion times, tens of billions of times and trillions of times more than that of the sun. Like the Milky Way, galaxies are also composed of stars and gases. Three, five, ten, dozens or even hundreds of thousands of galaxies form a galaxy group, called Galaxy cluster Galaxy cluster

classification

Announce
edit
Astrophysics
Astrophysics from research method Can be divided into Measured astrophysics And theoretical astrophysics. The former studies the basic observation technology in astrophysics, the principle and structure of various instruments and equipment, and the analysis and processing of observation data, so as to provide data or test for theoretical research theoretical model Optical astronomy It is an important part of measured astrophysics. The latter is based on the observation data theoretical analysis , establish a theoretical model to explain various astronomical phenomena. At the same time, it can also predict the celestial bodies and phenomena that have not yet been observed.
It is mainly classified according to the research object classification method , can be divided into:

Heliology

Astrophysics
To study various phenomena on the solar surface Inside the Sun Structure, energy source, chemical composition, etc. The sun is closely related to the earth. Studying the influence of the sun on the earth is also an important aspect of solar physics.
Study various celestial bodies in the solar system except the sun, such as planets, satellites asteroid , meteor Meteorite Comet. Interplanetary matter The nature, structure, chemical composition, etc.

Stellar science

To study the nature, structure, physical condition, chemical composition, origin and evolution of various stars. There are 100 billion or 200 billion stars in the Milky Way, and their physical conditions vary greatly. Some stars have very special conditions, such as Ultrahigh temperature Ultrahigh pressure , ultra-high density Super magnetic field Wait, these conditions are not available on earth. It is an important task of stellar physics to explore physical laws by using special physical conditions on stars.
④ Stellar astronomy
To study the spatial distribution of stars, star clusters, nebulae, interstellar matter, etc. in the Milky Way Kinematic characteristics To further explore the structure and nature of the Milky Way.

Galactic science

also called Extragalactic astronomy , studying galaxies (including the Milky Way), galaxy clusters Intergalactic space The form, structure, movement, composition physical property Etc.

Cosmology

⑦ Cosmology
Study the structure and evolution of the universe from a holistic perspective. Including focusing on the discovery of the universe large scale Observational characteristic Observational cosmology And focusing on the study of the universe kinematics And dynamics and building Cosmic model The theoretical cosmology of.
Astrophysics
To study the origin and evolution of celestial bodies. The research on the origin and evolution of the solar system started early. Although many important achievements have been made, no theory has been considered perfect and generally accepted. Stellar sample Rich and colorful , great progress has been made in the research on the origin and evolution of stars Evolutionary theory It has been widely accepted. yes Origin of galaxies And the research of evolution is still in the exploratory stage.
The various branches of astrophysics are interrelated and cross cutting.
With new technologies, new methods New theory Some new branches of astrophysics have emerged, such as Radio astronomy Infrared astronomy Ultraviolet astronomy X-ray astronomy Etc. Astrophysics and other disciplines also cross and penetrate each other. Some cross disciplines have also emerged, such as Astrochemistry Astrobiology Etc.

Other disciplines

⑩ Radio astronomy
Radio astronomy is studied by observing radio waves of celestial bodies Astronomical phenomenon A subject of. because Earth's atmosphere The radio waves from celestial bodies can reach the ground only when the wavelength is about 1mm to 30m. So far, most radio waves Astronomical research All are carried out in this band. Radio astronomy uses radio reception technology as the observation means, and the objects observed cover all celestial bodies: celestial bodies To all kinds of objects in the Milky Way, and to targets far away from the Milky Way. Radioastronomical radio technology It really began to develop in the 1940s.
Through on Upper atmosphere And atmosphere outer space conduct Astronomical exploration The discipline of collecting data and conducting astronomical research. Astronomy and space science It is a marginal discipline. Celestial objects are constantly emitting R ray X-ray , UV visible light infra-red Radio wave Equiwavelength electromagnetic wave , but only visible light and Near infrared light , near ultraviolet , 1 mm to 30 m radio waves, and several short wavelength ranges in the infrared wave band radiant energy Reaching the ground, the rest are Atmospheric absorption Or reflected. After the artificial satellite was launched, people were able to completely overcome the barrier of the earth's atmosphere and began to observe the whole electromagnetic band of celestial bodies, resulting in Space astronomy The birth of. Space astronomy uses high-altitude aircraft stratosphere Balloon Sounding rocket Artificial earth satellite Interplanetary probe spacecraft Etc Means of delivery
After the 1960s, yes celestial bodies The space exploration achievements of Apollo spacecraft Six times to send astronauts Moon , carried out on-the-spot investigation The interplanetary probe has repeatedly realized Mercury , Venus, Mars Jupiter Saturn Uranus and Neptune And made many important discoveries Interplanetary space About solar wind Interplanetary medium Interplanetary magnetic field A large amount of valuable information.
A branch of astrophysics. The main task is to study various high-energy phenomena and processes occurring on celestial bodies. It covers a wide range, including High-energy particle (or High-energy photon )Various astronomical phenomena and physical process It also includes astronomical phenomena and physical processes that generate and release a lot of energy. At the earliest time, high-energy astrophysics was mainly limited to the detection and research of cosmic rays. It was really established as a discipline after the 1960s.
After the 1960s, various new detection methods were applied to Astronomical research The discovery of a large number of new celestial bodies and phenomena has led to the rapid development of high-energy astrophysics. The research objects of high-energy astrophysics include quasars and activities Galactic nucleus , pulsar Supernova explosion , black hole theory X-ray source Gamma ray source , cosmic rays, various neutrino Processes and high-energy particle processes.
Astrophysics
In addition, there are also some high-energy processes on some celestial bodies, such as quasars and pulsars. They are High-energy astrophysics The research object of. High energy astrophysics has made some important achievements in the following aspects: Possible Has made groundbreaking research on the neutrino process of Photoneutrino process Electron pair Annihilation neutrino process and Neutrino process in plasmon decay It has important influence on the evolution of late stars; yes Solar neutrino There is a big gap between the experimental value and the theoretical value; about Supernova The mechanism of the outbreak of the proposed a promising theory; Supernova explosion may be the main source of cosmic rays; Some energies greater than 10 are detected in cosmic rays Electron volt In 1972, the Yunnan Station of the Institute of Atomic Energy of the Chinese Academy of Sciences found a particle with a mass of more than 1.8 × 10 grams Charged Particles; find Galactic nucleus The outbreak of the phenomenon and intense activity.

research meaning

Announce
edit
The expanding understanding of the universe not only makes people more and more deeply understand the structure and evolution of the universe, but also makes physics reveal Microcosm We have made progress in the mystery of. helium The element was first found on the sun, and it took more than 20 years to find it on the earth. heat nuclear fusion The concept was proposed in the study of star energy. Due to the limitation of ground conditions, the verification of some physical laws can only be carried out through the "laboratory" of the universe.
Four major discoveries in astronomy in the 1960s: quasars, pulsars, interstellar molecules and microwaves Background radiation , promoting high-energy astrophysics, cosmochemistry, astrobiology and Astrochemistry The development of the science of physics, chemistry and biology has also raised new topics.