Flarestar Observatory

Last updated
Flarestar Observatory
Observatory code 171 Blue pencil.svg
Location San Gwann, Malta
Coordinates 35°54′40″N14°28′15″E / 35.9111°N 14.4708°E / 35.9111; 14.4708 Coordinates: 35°54′40″N14°28′15″E / 35.9111°N 14.4708°E / 35.9111; 14.4708
Altitude 126 m [1]
Established 1999
Website http://flarestar.weebly.com
Telescopes
Meade SSC-10 0.25-m Schmidt-Cassegrain [2]
Malta relief location map.png
Red pog.svg
Location of Flarestar Observatory

Flarestar Observatory (obs. code: 171) is an astronomical observatory owned and operated and managed by astronomer and AAVSO-member Stephen M. Brincat. It is located near San Ġwann on the island country of Malta.

Since its founding in 1911, the American Association of Variable Star Observers (AAVSO) has coordinated, collected, evaluated, analyzed, published, and archived variable star observations made largely by amateur astronomers and makes the records available to professional astronomers, researchers, and educators. These records establish light curves depicting the variation in brightness of a star over time.

San Ġwann Local council in Central Region, Malta

San Ġwann is a town in the Central Region of Malta, with a population of 12,523 as of March 2014. Previous to its separate administration the town used to form part of two separate localities being Birkirkara and St. Julians.

Malta island republic in Europe

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The observatory's principal instrument is a Meade 0.25-meter aperture Schmidt-Cassegrain Telescope (SCT), which is routinely employed for photometric observations of asteroids and monitoring variable stars.

Photometry is a technique of astronomy concerned with measuring the flux, or intensity of an astronomical object's electromagnetic radiation. When photometry is performed over broad wavelength bands of radiation, where not only the amount of radiation but also its spectral distribution is measured, the term spectrophotometry is used.

Asteroid Minor planet that is not a comet

Asteroids are minor planets, especially of the inner Solar System. Larger asteroids have also been called planetoids. These terms have historically been applied to any astronomical object orbiting the Sun that did not resemble a planet-like disc and was not observed to have characteristics of an active comet such as a tail. As minor planets in the outer Solar System were discovered they were typically found to have volatile-rich surfaces similar to comets. As a result, they were often distinguished from objects found in the main asteroid belt. In this article, the term "asteroid" refers to the minor planets of the inner Solar System including those co-orbital with Jupiter.

Variable star star whose brightness as seen from Earth fluctuates

A variable star is a star whose brightness as seen from Earth fluctuates.

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References

  1. Flarestar Observatory
  2. Observatory - Flarestar Observatory official page