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Latest Info
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CLICK HERE - Viewing Situation
at the Briars Viewing
Centre

 

Horsehead - TSA102S

Horsehead & Flame Nebula Region

The Horsehead Nebula (also known as Barnard 33' in bright nebula IC 434) is a dark nebula in the Orion constellation. The nebula is located just below Alnitak, the easternmost star of Orion's Belt, and is part of the much larger Orion Molecular Cloud Complex. It is approximately 1,500 light years from Earth, and is approximately 3.5 light years wide.

One of the most identifiable nebulae in the sky, it is part of a swirling cloud of dark dust and gases, shaped like a horse's head (hence its name). Also known as Barnard 33, the unusual shape was first discovered in 1888 by Mrs. Williamina Fleming on photographic plate B2312 taken at the Harvard College Observatory.

The red glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left. Streams of gas leaving the nebula are funneled by a strong magnetic field. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming. 
(From Wikipedia, the free encyclopedia)

The Flame Nebula, designated as NGC 2024, is in the Constellation Orion. It is about 900 to 1,500 light-years away.

The bright star Alnitak (ζ Ori), the easternmost star in the Belt of Orion, shines energetic ultraviolet light into the Flame and this knocks electrons away from the great clouds of hydrogen gas that reside there. Much of the glow results when the electrons and ionized hydrogen recombine. Additional dark gas and dust lies in front of the bright part of the nebula and this is what causes the dark network that appears in the centre of the glowing gas. The Flame Nebula is part of the Orion Molecular Cloud Complex, a star-forming region that includes the famous Horsehead Nebula.

(From Wikipedia, the free encyclopaedia)

Exposure Data

bulletInstrument: Takahashi TSA102S (TOA Reducer/ Flattener)
bulletF/stop: 5.8
bulletExposure:
bulletCamera: Hutech Canon EOS 40D DSLR
bulletSensitivity: ISO 1600
bulletMount: Skywatcher EQ6 Pro
bulletDate: November 29, 2008
bulletExposure start:
bulletLocation: Heathcote, Victoria
bulletAutoguider: none
bulletEnhancement: Registar 1.0, Adobe Photoshop CS2,
bulletNotes: Guiding PHD

 
Up
Eta Carinae - TSA102S
Horsehead - TSA102S
Omega Centauri - ED80
Orion M42 - TSA102S
M33 - TSA102S
M45 - TSA102S
NGC2070 - TSA102S
M8 - TSA102S
M16 - TSA102S
M17 - TSA102S
M27 - TSA102S
M57 - TSA102S
Veil Nebula - TSA102S
NGC253 - TSA102S
M20 - VC200L
NGC2070 - VC200L
NGC5128 - VC200L
Rosette Nebula - TSA102S
M31, M101, M32 - TSA102S
M20 & M8 - TSA102S
M17 - VC200L

Public Viewing Nights 

Just to let everyone know, public viewing nights are held every first Friday of the month. Clear or cloudy nights the public viewing night goes ahead. Members man a number of telescopes of various sizes and types, and for those nights where the sky is cloudy, extended astronomical presentations are presented in the MPAS Viewing Centre.

So please come along and enjoy our nights sky.

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