Leeds Astronomical Society LAS Meetings Observing Membership

 

 

M42 - Orion Nebula

(James Clark)
(Ivor Trueman)

Information...

M42 - the Orion Nebula is a splendid diffuse nebula in the Milky Way. Located at a distance of 1,344 light years, it is the closest region of massive star formation to Earth. It is estimated to be 24 light years across and has approx. 2,000 × the mass of the Sun.

The nebula contains a very young open cluster, referred to as the Trapezium, due to an asterism of four bright stars. This cluster, which actually contains more than 300 very young stars, is responsible for the ionisation of surrounding gas, which gives rise to it's colourful nature in photographs.

The red hue is a result of recombination of Hydrogen II atoms, with a wavelength of 653nm, whilst green observed is caused by electron transistions in doubly ionised Oxygen.

Spectroscopic analysis of the nebula has revealed the prescence of many complex organic compounds in the nebula including:- Methanol, Hydrogen Cyanide, Sulphur Dioxide, Hydrogen Sulphide, Formyl Cation, Formaldehyde, Dimethyl Ether, Water, Carbon Monoxide, Acrylonitrile and Methyl Formate.

In James Clark's image above, the Running Man nebula can also be seen on the left of M42. This is a reflection nebula 1,460 light years away, and is actually comprosed of three nebulae: NGC1973, NGC1875 & NGC1977.

For more info. see the Wikipedia entry.

 

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Map

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Measuring Angles

Hold your arm at full length, then close one eye & use the hand shapes shown above to measure the angular distance between the stars.

(Ain't anatomy wonderful!)

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Apparent Magnitude

The apparent magnitude of a star is a measure of how bright it appears from Earth. The scale was introduced over 2,000 years ago by the Greek astronomer Hipparchus, who grouped stars into six categories. The brightest 20 or so were deemed to be 'first magnitude', slightly dimmer stars 'second magnitude', and so on until the barely visible stars were classed as 'sixth magnitude'.

Later it was recognised that our eyesight, once it has been given time to get used to darkness, has a logarithmic response. i.e. a Mag. 1 star is actually 2.512 times brighter than a Mag. 2 star, or 6.310 times brighter than a Mag. 3 star (2.512 x 2.512 = 6.310).

The six Magnitudes thus corresponds to a 2.5126 difference in brightness or 100x.

Apparent magnitude

Today the scale has now been extended, so that brighter objects can have an apparent magnitude of 0 or even negative. The brightest star Sirius, for example, has an apparent magnitude of -1.44 and the Sun is a whopping -26.74, due to it's close proximity to Earth.

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Diffuse Nebula

Diffuse Nebula is a term given to clouds of interstellar gas & dust which do not have well defined boundaries. If the clouds are large and massive enough they are frequently places of new star formation, with associations or clusters of stars. If the stars formed are large enough, and emit sufficient radiation to ionise the surrounding gas & cause it to shine, then the nebula is called an emission nebula. These are usually dominated by a red hue, from the recombination of Hydrogen II. On the other hand if the stars are not hot enough to create ionisation, their light is seen as scattering off the dust & gas creating a reflection nebula with a white or blue-ish hue.

Sometimes regions of both emission and reflection can be seen in the same nebula, for example in the Triffid Nebula shown below. (This image was taken by a LAS member using the free Open University remote telescope 'COAST' in Teneriffe.)

M20 - Triffid Nebula
M20 - Triffid Nebula (OU COAST scope)

The clouds of gas and dust will after a few million years, have all been used up in forming new stars and planets, or blown away by the stellar wind from the newly formed stars. Once that has happened, only the open cluster formed by those stars will be visible.

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