Examples of using Variable star in English and their translations into German
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Colloquial
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Official
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Ecclesiastic
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Medicine
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Financial
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Ecclesiastic
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Political
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Computer
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Programming
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Official/political
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Political
Variable star delta Cap.
References====External links==* AAVSO Variable Star of the Month.
The variable star EW CMa.
Light Curve produced by the American Amateur Variable Star Observers.
The variable star UW CMa.
R Hydrae, also known as R Hya, is a Mira-type variable star in the constellation Hydra.
The variable star RZ Cassiopeiae.
This pulsing led astronomers to mistake the system for a variable star for a long time.
Variable star kappa Pav period: 9 days.
Chi Cygni(χ Cyg, χ Cygni) is a variable star of the Mira type in the constellation Cygnus.
Variable star beta Peg period:~35 days.
This globular cluster has the third rank in known variable star population, after M3 and Omega Centauri;
A variable star brightens and dims over time.
He returned to Marengo, Illinois where he kept a small, private observatory that he used primarily for variable star observation.
The variable star eta Aql is one of the brightest Cepheids;
Shortly before he retired, he succeeded in detecting technetium in the variable star R Andromedae and other red variables. .
The variable star TX Psc(19 Psc) shows a deep red color spectral type C5III.
The AAVSO is an association formed by amateur astronomers that collect, evaluate, analyse, publish and archive variable star observations.
It is the brightest variable star in the sky, and therefore the most studied.
March 22, 2004 was a Turkish-Americanastronomer who was the director of the American Association of Variable Star Observers(AAVSO) from 1973 to 2004.
The brightness of the variable star rho Per varies semiregularily from 3rd mag to 4th mag.
Several observatories contributed to follow-up activities through the"Red Dots" project,including observers from the AAVSO American Association of Variable Star Observers.
Mu Cephei is a variable star and the prototype of the class of the Mu Cephei variables. .
Opens the AAVSO Light Curve Generator Tool, which allows you to download a lightcurve for any variable star from the American Association of Variable Star Observers.
With the variable star speed and the hydraulically adjustable screen deck angle, this system can be adapted to varying input qualities at the touch of a button and yields precise and classifiable output at all times.
Leavitt was a member of Phi Beta Kappa, the American Association of University Women, the American Astronomical and Astrophysical Society, the American Association for the Advancement of Science,and an honorary member of the American Association of Variable Star Observers.
The variable star eta Car behaves most erratically: In 1843 it flared up to a maximum brightness of -1 mag(which comes close to Sirius(alpha CMa)), but nowadays it shines as a 6th or 7th mag star. .
Fainter than: Sometimes the star is too faint to be seen by the observer. When that happens, the observer reports the faintest star seen in the field.These are called fainter thans because the variable star was fainter than the brightness reported.
Kstars; can display light curves for variable stars from the observing program of the American Association of Variable Star Observers(AAVSO). This program monitors over 6,000 variable stars and consists of 10 million observations going back almost a century.& kstars; downloads the very latest data directly from the AAVSO database via the Internet, so a network connection is required to use this tool.
To use the tool, select a variable star either by designation or name in the left panel, and set the start and end dates to be plotted. In the right panel, select the type of data that should be plotted(see below). When you have made you selections, press the Retrieve Curve button.& kstars; will automatically connect to the AAVSO server, which will generate the lightcurve plot and send it to your computer for display. A sample lightcurve plot is shown below.