NGC 246 Skull Nebula Captured from Pearly Bea...
NGC 246 (also known as the Skull Nebula or Caldwell 56) is a planetary nebula in the constellation Cetus (The Whale), discovered by William Herschel in 1785.
Gansbaai offers fine dining, superb accommodation, fantastic outdoor activities such as horse trails with Gansbaai & Pearly Beach Horse Trails, shark cage diving, walking trails and much more, as well as great unpolluted night skies.
You don't have to go all the way to cold Sutherland for stargazing. Southern Cape Astronomy offers Night Sky Safaris from their observatory just outside Pearly Beach. A selection of telescopes from 8” to 12” are used as well as video cameras for live views through the telescopes. The club also offers an evening of stargazing (at Pearly Beach Village Green), where all are welcome, normally on the closest Saturday to the New Moon each month.
Over the New Moon period in May, Southern Cape Astronomy hosted a well-attended stargazing evening a the Village Green in Pearly Beach. Deepsky objects such as Centaurus A, the Jewel Box, the Great Orion Nebula, Leo Triplet and Sombrero Galaxy amongst many others were looked at. Two of the giant gas planets, Jupiter & Saturn, were also visible, and Saturn with its icy ring system brought out many oohs and aahs.
One of the highlights during this period of clear skies was the close approach of the “lost asteroid”. This chunk of rock with a diameter of between 60-130 meters, whizzed past us at half the distance to the Moon on Tuesday 15th May. At closest approach (203 000 km, 0.55 lunar distance at a relative velocity of 12.8 km/s) the asteroid shone like an 11th magnitude star. Known as the “lost asteroid” (because astronomers lost track of it after its discovery in November 2010), its formal designation is 2010 WC9. The asteroid is in the same class as the Tunguska impactor which levelled a forest in Siberia in 1908.
The 12inch (for observations) and the 8 inch (imaging) were used during the asteroid's close approach.
The Apollo type NEO (near-Earth object) was discovered by the Catalina Sky Survey (Tuscon, Arizona), on the 30th October 2010. Observed through to December of that year, the asteroid reached an apparent magnitude of +21.8 and was becoming too faint to track. The asteroid has a perihelion of 0.77 AU and an Aphelion of 1.37 AU, an orbital period of 1.12 years, with a rotational period of 8 – 20 minutes.
Image marked 2010 WC9 near B59 Asteroid taken on15/05/2018 @ 18:34 UT, is one 30 second light frame, Canon 60D with 200mm lens working at f2.8, ISO 3200. The bright star on the left-hand side of the image is the globular cluster M19. Field of view is 4.91 x 3.96 degrees. Image marked 20 x 30 shows the asteroid's movement over a 10 minute period.
