ASTRONOMICAL SOCIETY: OCTOBER 2012
Weather permitting; we will meet on Thursday, 18th October, 6.30 p.m. at Pedro Castle.
If the sky is more than 50% cloud covered, we cancel. This can be, as you will appreciate, a sometimes difficult decision.
Almost directly overhead at viewing time is the constellation Aquila. Aquila lies just a few degrees north of the celestial equator and is located along the Milky Way. Because of this location along the line of our galaxy, many clusters and nebulae are found within its borders, but they are dim and there are few galaxies.
Astronomers observed two major novae in Aquila, the first one being in 389 BC. It was recorded as brighter than the planet Venus. The second one was observed in the year 1918 (Nova Aquilae). It was brighter than Altair. A nova should not be confused with a supernova. A nova is an old star that brightens temporarily, and a supernova (dying star) is a massive star exploding. NASA’s Pioneer 11 mission will pass near one of constellation Aquila’s stars in about four million years. Altair (Alpha Aquila), the brightest star of the constellation, is a multiple star system. It is about eight times brighter than the sun and the twelfth brightest star in the night sky. It is an A-type main sequence star with an apparent visual magnitude of 0.77. Class A stars are among the more common naked eye stars, and are white or bluish-white. Other examples include Sirius, Deneb, Vega and Fomalhaut. Altair is located 16.7 light-years (5.13 parsecs) from Earth and is one of the closest stars visible to the naked eye. Altair is a type-A main sequence star with approximately 1.8 times the mass of the Sun and 11 times its luminosity. Altair possesses an extremely rapid rate of rotation; it has a rotational period of approximately 9 hours. For comparison, the equator of the Sun requires just over 25 days for a complete