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Stellar and Astrometric

Webpages concerning "Stellar and Astrometric"

A database of online spectra from 3600 nearby stars, including photometry, and astrometry
http://stellar.phys.appstate.edu
Keywords:
NStar, Nstar, nearby, star, stars, spectra, spectrum, Online, Spectra, MK, standard, standards, NASA, stellar, neighborhood

http://stellar.phys.appstate.edu

THE 50 NEAREST STARS :This table contains all the 50 known stars within 4.9 parsecs of the Sun. For each star, this list contains the trigonometric parallax, distance to the Sun ( in light years and in parsecs ), visual and absolute magnitude, proper motion, spectral type, coordinates and constellation..
http://www.cosmobrain.com/cosmobrain/res/nearstar.html
Keywords:
nearest star, NEAREST STARS, near star, near stars, STARS, STAR, NEAREST, NEAR, SOLAR SYSTEM, SUN, alpha centauri, BARNARD'S STAR, BARNARD STAR, parallax, TRIGONOMETRIC PARALLAX, PARALLAXES, PARSEC, PARSECS, SIRIUS, EXOPLANETS, extra-solar, nearest star, NEAREST STARS, near star, near stars, STARS, STAR, NEAREST, NEAR, SOLAR SYSTEM, SUN, alpha centauri, BARNARD'S STAR, BARNARD STAR, parallax, ...

http://www.cosmobrain.com/cosmobrain/res/nearstar.html

Double Star Library
http://ad.usno.navy.mil/wds/dsl.html

http://ad.usno.navy.mil/wds/dsl.html

http://archive.ast.cam.ac.uk/hipp/hipparcos.html

http://archive.ast.cam.ac.uk/hipp/hipparcos.html

http://procyon.lpl.arizona.edu/WD/

http://procyon.lpl.arizona.edu/WD/

http://adc.gsfc.nasa.gov/adc/adc_cat1_holdings.html

http://adc.gsfc.nasa.gov/adc/adc_cat1_holdings.html

http://arch-http.hq.eso.org/gsc/gsc-query2.html

http://arch-http.hq.eso.org/gsc/gsc-query2.html

http://www.willbell.com/software/hypersky/wd1987.htm

http://www.willbell.com/software/hypersky/wd1987.htm

http://www.nofs.navy.mil/projects/pmm/catalogs.html

http://www.nofs.navy.mil/projects/pmm/catalogs.html

http://astro.estec.esa.nl/Hipparcos/

http://astro.estec.esa.nl/Hipparcos/

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Wikipedia-Article "Stellar"

Look up stellar in Wiktionary, the free dictionary.

Typically, stellar is an adjective referring to one or more stars. See also:

This article is based on the article "Stellar" from Wikipedia - the free encyclopedia created and edited by online user community. This article is distributed under the terms of GNU Free Documentation License. Here you find the list of authors of this article. The article can only edited within Wikipedia. Edit this article in Wikipedia.

Wikipedia-Article "Astrometric"

Illustration of the use of optical wavelength interferometry to determine precise positions of stars.  Courtesy NASA/JPL-Caltech.
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Illustration of the use of optical wavelength interferometry to determine precise positions of stars. Courtesy NASA/JPL-Caltech.

Astrometry is a branch of astronomy that deals with the positions of stars and other celestial bodies, their distances and movements.

It is one of the oldest subfields of the science, the successor to the more qualitative study of positional astronomy. Astrometry dates back at least to Hipparchus, who compiled the first catalogue of stars visible to him and in doing so invented the brightness scale basically still in use today. Modern astrometry was founded by Friedrich Bessel with his Fundamenta astronomiae, which gave the mean position of 3222 stars observed between 1750 and 1762 by James Bradley.

Apart from the fundamental function of providing Astronomers with a reference frame to report their observations in, astrometry is also fundamental for fields like celestial mechanics, stellar dynamics and galactic astronomy. In observational astronomy, astrometric techniques help identify stellar objects by their unique motions. It is instrumental for keeping time, in that UTC is basically the atomic time synchronized to Earth's rotation by means of exact observations. Astrometry is also involved in creating the cosmic distance ladder because it is used to establish parallax distance estimates for stars in the Milky Way.

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Advances in astrometry

Astronomers use astrometric techniques for the tracking of near-Earth objects. It has been also been used to detect extrasolar planets by measuring the displacement they cause in their parent star's apparent position on the sky, due to their mutual orbit around the center of mass of the system. NASA's planned Space Interferometry Mission (SIM PlanetQuest) will utilize astrometric techniques to detect terrestrial planets orbiting 200 or so of the nearest solar-type stars.

Astrometric measurements are used by astrophysicists to constrain certain models in celestial mechanics. By measuring the velocities of pulsars, it is possible to put a limit on the asymmetry of supernova explosions. Also, astrometric results are used to determine the distribution of dark matter in the galaxy.

Astrometrics

Astrometrics is the science of stellar measurements and motion. Astrometrics was used, during the 1990s, to detect extrasolar gas giants orbiting various solar systems. This was done by observing the "stellar wobble" of a star and calculating what kinds of gravitational forces would cause such motion; it was then determined that planetary forces must be affecting the stars in question.

Other references

In the fictional Star Trek: Voyager, the Astrometrics lab is the set for various scenes.

See also


General subfields within astronomy

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Astrometry | Astrophysics | Cosmology | Galactic astronomy | Extragalactic astronomy | Galaxy formation and evolution | Planetary science | Stellar astronomy | Stellar evolution | Star formation
This article is based on the article "Astrometric" from Wikipedia - the free encyclopedia created and edited by online user community. This article is distributed under the terms of GNU Free Documentation License. Here you find the list of authors of this article. The article can only edited within Wikipedia. Edit this article in Wikipedia.