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Jump to navigationJump to searchNew page: ===Astronomy=== This discipline is the science of celestial objects and phenomena that originate outside the Earth's atmosphere. It is concerned with the e...
===Astronomy===
This discipline is the science of [[Astronomical object|celestial objects]] and [[phenomena]] that originate outside the [[Earth's atmosphere]]. It is concerned with the evolution, [[physics]], [[chemistry]], [[meteorology]], and [[motion (physics)|motion]] of celestial objects, as well as the [[physical cosmology|formation and development of the universe]]. Astronomy includes the examination, study and modeling of [[star]]s, [[planet]]s, [[comet]]s, [[galaxy|galaxies]] and the [[cosmos]]. Most of the information used by astronomers is gathered by remote observation, although some laboratory reproduction of celestial phenomenon has been performed (such as the molecular chemistry of the [[interstellar medium]].)
While the origins of the study of celestial features and phenomenon can be traced back to antiquity, the scientific methodology of this field began to develop in the middle of the seventeenth century. A key factor was [[Galileo Galilei|Galileo]]'s introduction of the telescope to examine the night sky in more detail. The mathematical treatment of astronomy began with [[Isaac Newton|Newton]]'s development of [[celestial mechanics]] and the laws of [[gravitation]], although it was triggered by earlier work of astronomers such as [[Johannes Kepler|Kepler]]. By the nineteenth century, astronomy had developed into a formal science with the introduction of instruments such as the [[spectroscope]] and [[photography]], along with much improved telescopes and the creation of professional observatories.
[[Category: General Reference]]
This discipline is the science of [[Astronomical object|celestial objects]] and [[phenomena]] that originate outside the [[Earth's atmosphere]]. It is concerned with the evolution, [[physics]], [[chemistry]], [[meteorology]], and [[motion (physics)|motion]] of celestial objects, as well as the [[physical cosmology|formation and development of the universe]]. Astronomy includes the examination, study and modeling of [[star]]s, [[planet]]s, [[comet]]s, [[galaxy|galaxies]] and the [[cosmos]]. Most of the information used by astronomers is gathered by remote observation, although some laboratory reproduction of celestial phenomenon has been performed (such as the molecular chemistry of the [[interstellar medium]].)
While the origins of the study of celestial features and phenomenon can be traced back to antiquity, the scientific methodology of this field began to develop in the middle of the seventeenth century. A key factor was [[Galileo Galilei|Galileo]]'s introduction of the telescope to examine the night sky in more detail. The mathematical treatment of astronomy began with [[Isaac Newton|Newton]]'s development of [[celestial mechanics]] and the laws of [[gravitation]], although it was triggered by earlier work of astronomers such as [[Johannes Kepler|Kepler]]. By the nineteenth century, astronomy had developed into a formal science with the introduction of instruments such as the [[spectroscope]] and [[photography]], along with much improved telescopes and the creation of professional observatories.
[[Category: General Reference]]
