Chris Rowlands Observer Information

Observing Information for the Waddesdon Star Party, 1st March 2014

Jupiter

Jupiter is the biggest planet in our solar system and shows a disk with even the smallest telescope.  Better scopes will show two dark cloud bands, with the Great Red Spot on the Southern edge of the southern band.  The Great Red Spot will be crossing the visible disk; it will appear in the centre at 21:59 UTC. It should be visible but may not be as obvious as it appears in images.

Three of the four bright Galilean moons are visible, Ganymede then Europa to the East and Callisto on the West. The fourth moon, Io, will be hidden behind Jupiter from 20:15 and will emerge from Jupiter’s shadow about 23:39.

Jupiter is about 5 times the distance of the Earth from the Sun and orbits the Sun in just under 12 years. It has a mass of 318 times that of the Earth and is about 11 times the diameter. It rotates about its axis in just less than 10 hours, the fastest of the major planets.

Castor

Castor is the brightest star in the constellation Gemini, telescopes show as a double star. The two visible stars orbit each other in about 467 years.  Each of these stars is itself a very close spectroscopic binary star.  There is also a faint companion; this companion is an eclipsing binary.  This makes a total of six stars.

The distance is about 51 light years.

Binary stars are important because measurements of their orbit period and speed can give their mass and that, with observations of their spectrum helps with theories of how stars form and develop.

Algieba: Gamma Leo

This is a binary star in the mane of Leo. The stars may appear to be different colours with the brighter one orange-red and the dimmer one greenish-yellow. They are 100 light years away and the stars orbit each other in about 600 years.

Alcor and Mizar

This is a visual double star; it is the middle star in the tail of the Big Dipper. Mizar is the brighter star and is visible as a binary star in telescopes. Each of these stars are a spectroscopic binary, Mizar A was the first star to be identified as such.  Alcor is also a binary star.

Sigma Orionis

This is a five star system below Alnitak, the left most star of Orion’s belt. The primary is a binary that’s a little too close for us to separate with our telescopes and there are four other stars. They were formed 2.5 million years ago as part of a young cluster of stars.

M45: The Pleiades

The Pleiades is an open cluster of stars, easily visible with the naked eye.  The stars we see are the brightest ones of 1000 stars that were formed from a cloud of gas and dust about 100 million years ago.  As time passes the stars will go their separate ways and the cluster will dissipate.  This is expected to take about 250 million years.  The distance to the cluster is 390 to 460 light years and the central region is about 16 light years across.  Open clusters such as this are important for astronomy because they give a snapshot of stars of different masses, all at similar distances and of the same age.

M44: The Beehive

This is an open cluster of stars in the centre of the constellation Cancer, between Gemini and Leo.  It’s visible as a faint grey blob with dark skies.  The cluster formed about 600 million years ago and is about 520 to 610 light years away.  The centre is about 23 light years across and appears to be about three times the diameter of the Moon.  It’s older than the Pleiades so the bright high mass stars have come to the end of their lives and become white dwarfs.

Double Cluster

This is located to the NW, about half way up the sky.  This may be visible over the house.  It is two open clusters of stars close together in the Milky Way.  They seem to have formed together, about 12.8 million years ago and are both 7500 light years away.

M36, M37, M38

These three open clusters in Auriga are all high to the SW. They are 4 to 5 thousand light years away.

M46, M47

These are a couple of open clusters fairly low to the South.  M46 contains a planetary nebula.

M42: The Orion Nebula

This is a huge star forming region, made of a vast cloud of gas and dust. Stars are forming and some of the brighter ones are illuminating the centre of the cluster.  These show as the Trapezium.

It’s about 1,344 light years away and is visible to the naked eye as a fuzzy blob under the belt of Orion.  It is about 24 light years across and 2000 times the mass of the Sun.

NGC2392: Eskimo Nebula

This is a planetary nebula in Gemini. It is about 3,000 light years away.  Visually it shows as a fuzzy star.  We think that the Sun will form a similar planetary nebula at the end of its life, in 4 to 5 billion years.

M3

This is a globular cluster in Bootes, low to the E. It’s a cluster of about 500,000 stars, 33,900 light years away and 8 billion years old.

Kemble’s Cascade

This is a three degree chain of stars ending with a small open cluster.  It is high to the NW.

M82: Cigar Galaxy

This is located almost overhead in the NE.  It’s visible in telescopes as a fuzzy oval.  Its centre is a region where large numbers of stars are being formed.  A Supernova was discovered in M82 on the 21st January.  It may still be visible just to the side of the centre as a tiny star. The galaxy is about 12 million light years away so that’s when the supernova actually happened.  M81, Bode’s Nebula is nearby.  This is a large spiral galaxy.

M51: The Whirlpool Galaxy

This is also almost overhead near the tail of the Big Dipper. It is a face on spiral galaxy with a smaller companion.  Our small telescopes only show the core of the galaxy but images show the spiral arms.

M31: The Andromeda Nebula

This is currently fairly low in the NW.  It may not be visible because the house is in the way.  This is the closest large galaxy to us, about 2 million light years away.  It’s about 3 degrees across and the centre is visible to the naked eye in dark skies.  Telescopes show the central core, you need long exposure images to produce the spectacular images we all expect.

General Questions

What are these M numbers?

These objects were first catalogued by Charles Messier and his collaborators in France in 1771.  He was searching for comets and made a list of objects that looked like comets but were not.  There are a total of 110 Messier objects.

 

Where are the other Planets?

Mars and Saturn are morning objects; they will become visible earlier in the evening as the year goes on. Mars will be in opposition in just over a month on the 8th April. A good time to observe Mars will be in April and May. Saturn will be at opposition on the 10th May so will be visible from May to July.

Venus is an early Morning object, rising before the Sun.  It will be visible throughout the spring and summer.

Mercury will be visible in the early evening over the next few weeks, with the best opportunity on the 14th March.  It is low to the W and is best seen not long after sunset.  It’s difficult to see because it’s so low and in the twilight sky.