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Wikipedia

Portal:Astronomy

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Wikipedia portal for content related to Astronomy
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Introduction

A man sitting on a chair mounted to a moving platform, staring through a large telescope.
Percival Lowell observing Venus from the Lowell Observatory telescope in 1914

Astronomy is anatural science that studiescelestial objects and thephenomena that occur in the cosmos. It usesmathematics,physics, andchemistry in order to explain their origin and their overallevolution. Objects of interest includeplanets,moons,stars,nebulae,galaxies,meteoroids,asteroids, andcomets. Relevant phenomena includesupernova explosions,gamma ray bursts,quasars,blazars,pulsars, andcosmic microwave background radiation. More generally, astronomy studies everything that originates beyondEarth's atmosphere.Cosmology is a branch of astronomy that studies theuniverse as a whole.

Astronomy is one of the oldest natural sciences. The early civilizations inrecorded history made methodical observations of thenight sky. These include theEgyptians,Babylonians,Greeks,Indians,Chinese,Maya, and many ancientindigenous peoples of the Americas. In the past, astronomy included disciplines as diverse asastrometry,celestial navigation,observational astronomy, and the making ofcalendars.

Professional astronomy is split intoobservational andtheoretical branches. Observational astronomy is focused on acquiring data from observations of astronomical objects. This data is then analyzed using basic principles of physics. Theoretical astronomy is oriented toward the development of computer or analytical models to describe astronomical objects and phenomena. These two fields complement each other. Theoretical astronomy seeks to explain observational results and observations are used to confirm theoretical results.

Astronomy is one of the few sciences in which amateurs play anactive role. This is especially true for the discovery and observation oftransient events.Amateur astronomers have helped with many important discoveries, such as finding new comets. (Full article...)

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Herbig–Haro(HH) objects are bright patches ofnebulosity associated with newbornstars. They are formed when narrow jets of partiallyionised gas ejected by stars collide with nearby clouds of gas and dust at several hundred kilometers per second. Herbig–Haro objects are commonly found instar-forming regions, and several are often seen around a single star, aligned with itsrotational axis. Most of them lie within about oneparsec (3.26light-years) of the source, although some have been observed several parsecs away. HH objects are transient phenomena that last around a few tens of thousands of years. They can change visibly over timescales of a few years as they move rapidly away from their parent star into the gas clouds of interstellar space (theinterstellar medium or ISM).Hubble Space Telescope observations have revealed the complex evolution of HH objects over the period of a few years, as parts of the nebula fade while others brighten as they collide with the clumpy material of the interstellar medium.

First observed in the late 19th century bySherburne Wesley Burnham, Herbig–Haro objects were recognised as a distinct type ofemission nebula in the 1940s. The first astronomers to study them in detail wereGeorge Herbig andGuillermo Haro, after whom they have been named. Herbig and Haro were working independently on studies ofstar formation when they first analysed the objects, and recognised that they were a by-product of the star formation process. Although HH objects are visible-wavelength phenomena, many remain invisible at these wavelengths due to dust and gas, and can only be detected atinfrared wavelengths. Such objects, when observed in near-infrared, are called molecular hydrogenemission-line objects (MHOs). (Full article...)

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Credit: Boris Štromar

Andromeda is one of the 48constellations listed by the 2nd-centuryGreco-Roman astronomerPtolemy, and one of the88 modern constellations. Located north of thecelestial equator, it is named forAndromeda, daughter of Cassiopeia. Andromeda is most prominent during autumn evenings in theNorthern Hemisphere.

Astronomy News

21 November 2024 –
TheEuropean Southern Observatory announces that its astronomers inChile capture the first close-up image of astar outside theMilky Way.(The New York Times)
20 November 2024 –Discoveries of exoplanets
In a study published by theNature journal, astronomers announce the discovery ofIRAS 04125+2902 b, a newbornexoplanet. The discovery was made by Madyson Barber, a graduate student at theUniversity of North Carolina at Chapel Hill.(Nature)(ABC News)

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