Home >> Regional >> North America >> Mexico >> Science and Environment >> Astronomy


  Ancient Mayan
       


Daedalus, photographed by the crew of Apollo 11 as they circled the Moon in 1969. Located near the center of the far side of Earth's Moon, its diameter is about 58 miles (93 km).]]

Uranology (Greek: αστÏ?ονομία = άστÏ?ον + νόμος, astronomia = astron + nomos, literally, "law of the stars") is the science of celestial objects & phenomena that originate outside Earth's atmosphere, such as stars, planets, comets, galaxies, and the cosmic background radiation. These are caring by using a formation and development of the universe, the evolution & physical and chemical properties of celestial objects & a calculation of their motions. Astronomical observations are not sole relevant for uranology inside and of itself, however provide essential references for the verification of fundamental theories in physical science, like general relativity theory. Complementary to experimental uranology, theoretical astrophysics seeks to explain astronomic phenomena.

Uranology is one of a oldest sciences, by owning a scientific methodology existent at the instance of Ancient Greece and advanced observation techniques possibly good deal earliest (watch archaeoastronomy). Historically, amateurs develop contributed to numbers of significant astronomic discoveries, & uranology is one of a couple of sciences in which amateurs can still play an active role, especially in the discovery and observation of short-lived phenomena.

Uranology is does'nt to exist as confused by using astrology, which assumes that people's destiny & person affairs in a main come correlated to the apparent positions of astronomic objects in the sky -- although them fields part the most common origin, it is quite different; uranologist embrace the scientific method, while astrologist don't.

Divisions

Inside ancient Greece and other early civilizations, uranology consisted largely of astrometry, measuring positions of stars & planets in the sky. Late, a operate of Kepler and Newton, whose work led to the development of celestial mechanics, mathematically predicting the motions of celestial bodies interacting under gravity, & solar system objects in particular. Great deal of the effort around these 2 arewhen, when done largely by hand, is extremely machine-driven present, to the extent that it is seldom considered as independent disciplines any longer. Motions & positions of objects come today further well determined, & modern uranology is additional caring by using researching & understanding a actual physical nature and severity of ethereal objects.

Since a twentieth century, a field of broker uranology has split into observational astronomy and theoretical astrophysics. Although virtually all stargazer incorporate elements of two into their search, because of a different skills required, virtually all agency uranologist tend to specialize inside a single or even the more. information-based uranology is caring mostly by using getting data, which involves building & maintaining instruments & processing a outcomes; this branch is at days known as "astrometry" or even only when "astronomy". Theoretical astrophysics is caring in a main using ascertaining the data-based implications of different system, & involves working using computer or even analytic system.

A fields of learn can too become categorized within more ways. Categorization per vicinity of space under survey (e.g., Astronomical uranology, Planetary Sciences); by subject, like star formation or even even cosmology; or per method utilized for obtaining principles.

By subject or problem addressed

Planetary astronomy, or Planetary Sciences: a Mars. Photographed by Mars Global Surveyor, the long dark streak is formed by a moving swirling column of Martian atmosphere (with similarities to a terrestrial tornado). The dust devil itself (the black spot) is climbing the crater wall. The streaks on the right are sand dunes on the crater floor.]]

Astrometry: the learn of the position of objects in the sky & their changes of position. Defines a technique of co-ordinate utilized & a kinematics of objects in my galaxy. Astrophysics: a survey of natural philosophy of the universe, including the physical properties (luminosity, density, temperature, chemical composition) of astronomical objects. Cosmology: the learn of the origin of the universe & its evolution. A survey of cosmology is theoretical astrophysics at its big shell. Galaxy formation and evolution: the survey of the formation of the galaxies, & their evolution. Galactic astronomy: the survey of the structure & components of my galaxy & of more galaxies. Extragalactic astronomy: the survey of objects (in the main galaxies) outside my galaxy. Stellar astronomy: the survey of the stars. Stellar evolution: the survey of the evolution of stars from either their formation to their prevent as a prima remnant. Star formation: a survey of the affliction & processes that led to the formation of stars in the interior of flatulency clouds, & the run of formation itself. Planetary Sciences: the survey of the planets of the Solar System. Astrobiology: the survey of the advent & evolution of biological systems in the Universe.

More disciplines that can be considered section of uranology:

Archaeoastronomy Astrochemistry Astrosociobiology Astrophilosophy View a list of astronomical topics for a further thoroughgoing listing of astronomy-related web sites.

Ways of obtaining information

Inside uranology, information is mainly received from either a detection & analysis of weak & more forms of electromagnetic radiation. More cosmic rays come also found, & many experiments are designed to detect gravitational waves in the near new.

a traditional section of uranology is from the region of the electromagnetic spectrum observed:

Optical astronomy is the part of uranology that utilizes optical components (mirrors, lenses, CCD detectors and photographic films) to observe light from touching infrared to near ultraviolet wavelengths. Visible light astronomy (using wavelengths that can be found by having a eyes, astir 400 - 700 nm) falls midmost of this range. A usual thing is the telescope, with electronic imagers and spectrographs. Infrared astronomy deals with a detection & analysis of infrared radiation (wavelengths yearn than red weak). A usual thing is the telescope but using the detector which is sensitive to the infrared. Space telescopes are also wont to eliminate noise (electromagnetic interference) from either a atmosphere. Radio astronomy detects radiation of millimetre to decametre wavelength. A receivers come similar to victims utilized within radio broadcast transmission but lot further sensitive. Look at too Radio telescopes. High-energy astronomy includes X-ray uranology, gamma-ray uranology, & extreme UV (ultraviolet light) astronomy, besides when studies of neutrinos & cosmic rays.

Optical & radio astronomy may be performed sustaining ground-depending observatories, because the atmosphere is transparent at the wavelengths existence found. Infrared weak is heavy absorbed by water vapor, so infrared observatories develop to exist as located within high, dry pages or even in space.

A atmosphere is opaque at the wavelengths of X-ray astronomy, gamma-ray astronomy, UV astronomy and (except for a few wavelength "windows") Far infrared astronomy, so observations must exist as carried retired mostly from either balloons or space observatories. Mighty gamma rays can, even so become found per big air showers they produce, & a survey of cosmic rays can also exist as repute a branch of uranology.

History of astronomy

Extragalactic astronomy: gravitational lensing. This image shows several blue, loop-shaped objects that are multiple images of the same galaxy, duplicated by the gravitational lens effect of the cluster of yellow galaxies near the photograph's center. The lens is produced by the cluster's gravitational field that bends light to magnify and distort the image of a more distant object.

Around early days, uranology simply comprised a observation & predictions of the motions of the naked-eye objects. Aristotle said that a Globe was a center of the Universe & all about rotated as much as it within orbits that were hone circles. Aristotle got to exist as best because humans thought that Gloexist as experienced to be within a center by having all about rotating in the area of it because the wind would non scatter leaves, & birds would simply fly in 1 counsel. For an extended instance, population thought that Aristotle was perfect, however these are likely that Aristotle inadvertently did sir thomas more to hinder my noesis than support it. A Rigveda refers to the 27 constellations associated with a motions of a sun & besides the Twelve zodiacal divisions of the sky. A ancient Greeks made important contributions to uranology, among a children the definition of the magnitude system. A Bible contains a total of statements on a position of the globe in the universe & the nature & severity of the stars and planets, virtually all of which are then poetic like than literal; view Biblical cosmology. Within 500 AD, Aryabhata presented a mathematical formulwhen that described a globe as spinning in its axis & considered a motions of the planets using respect to the sun.

Data-based uranology was mostly stagnant within medieval Europe, but flourished in the Iranian world and more area of Islamic realm. A late 9th century Persian astronomer al-Farghani wrote extensively on the motion of celestial bodies. His act was translated into Latin in the 12th century. In the late 10th century, a immense observatory was built near Tehran, Persia (now Iran), by the Persian uranologist al-Khujandi, who found the series of meridian transits of the Sun, which allowed him to calculate the obliquity of the ecliptic. Likewise within Persia, Omar Khayyám performed a reformation of the calendar that was more exact than a Julian and came roughly a Gregorian. Abraham Zacuto was responsible in the 15th century for the adaptations of astronomical theory for the practical needs of Portuguese caravel expeditions.

In a period of the Renaissance, Copernicus proposed a heliocentric model of the Solar System. His act was defended, expanded upon, & disciplined by Galileo Galilei and Johannes Kepler. Galileo added a innovation of applying telescopes to enhance his observations. Kepler was a number 1 to devise a models that described aright a details of a motion of the planets by owning the Sun at the center. Even so, Kepler did non succeed within formulating a theory behind the laws he wrote down. It was left to Newton's invention of celestial dynamics and his law of gravitation to finally explain the motions of the planets. Newton as well developed a reflecting telescope.

Stars were encountered to become faraway objects. By using a advent of spectroscopy it was proved that they were similar to my have sun, however by using the wide range of temperatures, masses, and sizes. A being of my galaxy, the Milky Way, as a separate group of stars was just proven in the 20th century, along with a being of "external" galaxies, & shortly fallowing, a expansion of the universe, seen in the recession of most galaxies from either america. Modern uranology has besides found numbers of exotic objects like quasars, pulsars, blazars and radio galaxies, and has utilized these observations to evolve physical theories which describe a select few one objects within terms of equally exotic objects like black holes and neutron stars. Physical cosmology made huge advances when you took a 20th century, by using a model of the Big Bang heavily supported by a grounds to believe provided by uranology & natural philosophy, like the cosmic microwave background radiation, Hubble's Law, and cosmological abundances of elements.

Timelines in astronomy

Ant planetary nebula. Ejecting gas from the dying center star shows symmetrical patterns unlike the chaotic patterns of ordinary explosions.]]

Artificial satellites and space probes Astronomical maps, catalogs, and surveys Big Bang Black hole physics Cosmic microwave background astronomy Cosmology Galaxies, clusters of galaxies, and large scale structure Interstellar medium and intergalactic medium Natural satellites Other background radiation fields Solar astronomy Solar system astronomy Stellar astronomy Telescopes, observatories, and observing technology Universe White dwarfs, neutron stars, and supernovae

Astrophysical Plasmas: Codes, Models and Observations 1999.
International Conference organized by the Institute of Astronomy of the National University of Mexico (UNAM).

Institute of Astronomy at Morelia (UNAM)
Information about the researchers.

Instituto Nacional de Astrofisica, Optica y Electronica
The INAOE is a research and teaching institution specializing in astrophysics, optics, electronics, and computer sciences and offering post-graduate studies in these specialties.

Carl Sagan Observatory at Cerro Azul
Area de Astronomia of the Departamento de Investigacion en Fisica of the Universidad de Sonora. Programs, courses of study, infrastructure, news, activities and astrological events.

Eclipse Chaser's Journal: Total Solar Eclipse
Jeffrey R. Charles, an american astrophotographer, summarize his experiences in Mazatlan, Mexico, during the total solar eclipse of July 11th, 1991.

National Astronomic Observatory at San Pedro Martir
General information about the researchers and facilities of the Institute of Astronomy of the National University (UNAM) in Ensenada, Baja California.


Science: Astronomy






© 2005 GeneralAnswers.org