Leeds Astronomical Society LAS Meetings Observing Membership

 

 

NGC4631 - Whale Galaxy / NGC4656 - Crowbar Galaxy

(Ivor Trueman)
Cropped close-up (Ivor Trueman)
(James Clark)

Information...

NGC4631 is a barred spiral galaxy in the constellation of Canes Venatici. Viewed edge on from Earth, it's slightly distorted shape has earned it the nickname of the Whale or Herring galaxy.

Also in the NGC4631 galaxy group is NGC4656/NGC4657, a highly warped spiral galaxy. It's shape has led it to become known as the Crowbar or Hockey Stick galaxy.

The group is approx 25 million light years from Earth.

For more info. see the Wikipedia NGC4631 and NGC4656/57 entries.

 

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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.