Monday 11 August 2014

The Sky This Month

For an excellent review of what to look for in the night skies try this blog from the University of Manchester

http://www.jb.man.ac.uk/astronomy/nightsky/

Monday 3 February 2014

The night Sky - Feb 2014 C/O Ian Morison at the University of Manchester

The Night Sky February 2014

Compiled by Ian Morison

This page, updated monthly, will let you know some of the things that you can look out for in the night sky. It lists the phases of the Moon, where you will see the naked-eye planets and describes some of the prominent constellations in the night sky during the month.

Image of the Month

Supernova in M82

M82 Supernova

Image: Adam Block, Mt.Lemmon SkyCenter, University of Arizona.

A beautiful image of M82 taken by Adam Block showing the Type 1a supernova that was discovered by students at the University College London, Mill Hill Observatory, on the 21st January. M82 lies 12 million light years away in the constellation Ursa Major. Though it will be fading during February it should still be visible in a small telescope. A Type 1a supernova results when a white dwarf star accrets matter from a companion star. When the mass of the white dwarf exceeds the Chandrasekhar Limit (about 1.44 solar masses) when the star can no longer be supported by electron degeneracy pressure, it explodes. The peak brightness of a Type 1a supernova is believed to be constant and so these can be used as "standard candles" to determine the distances of remote galaxies. This has shown that the Universe is expanding at an increasing rate and is evidence for dark energy.

Highlights of the Month

February - a superb month to view Jupiter.

Jupiter imaged by Damian Peach

Following Jupiter's opposition on January 5th, this is a great month to observe Jupiter in the evening. It now lies Gemini and so is high in the ecliptic and hence, when due south, at an elevation of ~60 degrees and is high in the sky for most of the night. Jupiter's angular size remains at about 46 arc seconds throughout the month so a small telescope can see lots of details - surely one should be on your shopping list if you do not have one! It is looking somewhat different than in the last few years as the north equatorial belt has become quite broad. The Great Red Spot has recently become more prominent and can be easily seen as a large feature in the South Equatorial Belt.
The features seen in the Jovian atmosphere have been changing quite significantly over the last few years - for a while the South Equatorial Belt vanished completely (as seen in Damian's image) but has now returned to its normal wide state. The diagram on right shows the main Jovian features as imaged by the author at the beginning of December 2012. The highlight below gives the times when the GRS is facing us.
The image by Damian Peach was taken with a 14 inch telescope in Barbados where the seeing can be particularly good. This image won the "Astronomy Photographer of the Year" competition in 2011. See more of Damian Peach's images: Damian Peaches Website"

Features in Jupiter's atmosphere - December 2013.

February: Look for the Great Red Spot on Jupiter

Observe the Great Red Spot
Image: NASA

This list gives some of the best evening times during February to observe the Great Red Spot which should then lie on the central meridian of the planet.
1st 18:53 20th 19:33
3rd 20:31 22nd 21:12
5th 22:09 25th 18:42
8th 19:39 27th 20:20
13th 18:47
15th 20:25
17th 22:03

February 1st - after sunset: Mercury with a thin crescent Moon

Mercury with a thin crescent Moon
Image: Stellarium/IM

About 45 minutes after sunset on the night of the 1st of February and, given a low horizon in the southwest, one should be able to observe Mercury just below a thin crescent Moon. Mercury will be 50% illuminated. Try to observe the earthshine on the Moon - the "dark side" illuminated by the light reflected by clouds on Earth.

Earthshine : Ian Morison

February 10th - after sunset: Jupiter with a waxing Moon going towards full.

Jupiter and the Moon
Image: Stellarium/IM

Looking southeast after sunset on the evening of the 10th, Jupiter, in Gemini, will be seen seven degrees to the left of a waxing Moon.

February 19th - before dawn: Mars near a waning Moon

Image: Stellarium/IM

Before dawn on the 19th, Mars will be seen 5.5 degrees above Spica in Virgo and 10 degrees to the upper right of a waning Moon.

22nd February - late evening: spot Pallas - a large asteroid

Minor Planet Pallas
Image: Stellarium/IM

Minor planet (2), Pallas moves northwards through Hydra during February closing on the 2nd magnitude star Alphard as it does so. On the 22nd it reaches opposition - and will so be due south around midnight - shining at magnitude +7. That night it will lie 4 degrees away from Alphard so both will be seen in the same field of view of a pair of binoculars. Pallas is the second largest minor planet after Ceres in the main Asteroid Belt and is around 550 km across. On the 22nd it will it be just over twice as far from the Sun as the Earth. Incidently, should the diameter of an object be greater than 800 km, then gravity will make it spherical and it will now be classed as a dwarf planet. This is the case with Ceres.

February 26th - before dawn: Venus very close to a thin crescent Moon

Venus with a thin crescent Moon
Image: Stellarium/IM

Looking southeast before dawn on the morning of the 26th, Venus should be seen just half a degree above the disk of a slender waning crescent Moon. This should make a very good astrophotography target.

February 7th evening: The Hyginus Rille

Hyginus Rille location: IM.

For some time a debate raged as to whether the craters on the Moon were caused by impacts or volcanic activity. We now know that virtually all were caused by impact, but it is thought that the Hyginus crater that lies at the centre of the Hyginus Rille may well be volcanic in origin. It is an 11 km wide rimless pit - in contast to impact craters which have raised rims - and its close association with the rille of the same name associates it with internal lunar events. It can quite easily be seen to be surrounded by dark material. It is thought that an explosive release of dust and gas created a vacant space below so that the overlying surface collapsed into it so forming the crater.

Hyginus Crater and Rille

M109 imaged with the Faulkes Telescope

Messier 109
Image: Daniel Duggan
Faulkes Telescope North.

The Galaxy M109, imaged by Daniel Duggan.
This image was taken using the Faulkes Telescope North by Daniel Duggan - for some time a member of the Faulkes telescope team. It shows the barred spiral galaxy M109 that lies at a distance of 83 million light years in the constellation of Ursa Major. It is the brightest galaxy in the Ursa Major group of some 50 galaxies. Our own Milky Way galaxy is now thought to be a barred spiral like M109.
Learn more about the Faulkes Telescopes and how schools can use them: Faulkes Telescope"

Observe the International Space Station

The International Space Station and Jules Verne passing behind the Lovell Telescope on April 1st 2008.
Image by Andrew Greenwood

Use the link below to find when the space station will be visible in the next few days. In general, the space station can be seen either in the hour or so before dawn or the hour or so after sunset - this is because it is dark and yet the Sun is not too far below the horizon so that it can light up the space station. As the orbit only just gets up the the latitude of the UK it will usually be seen to the south, and is only visible for a minute or so at each sighting. Note that as it is in low-earth orbit the sighting details vary quite considerably across the UK. The NASA website linked to below gives details for several cities in the UK. (Across the world too for foreign visitors to this web page.)
Note: I observed the ISS three times recently and was amazed as to how bright it has become.
Find details of sighting possibilities from your location from: Location Index
See where the space station is now: Current Position

The Moon

The Moon at 3rd Quarter. Image, by Ian Morison, taken with a 150mm Maksutov-Newtonian and Canon G7.
Just below the crator Plato seen near the top of the image is the mountain "Mons Piton". It casts a long shadow across the maria from which one can calculate its height - about 6800ft or 2250m.

new moon	first quarter	full moon	last quarter
January 30th	February 6th	February 14th	February 22nd

Some Lunar Images by Ian Morison, Jodrell Bank Observatory: Lunar Images

A World Record Lunar Image

The 9 day old Moon.

To mark International Year of Astronomy, a team of British astronomers have made the largest lunar image in history and gained a place in the Guinness Book of Records! The whole image comprises 87.4 megapixels with a Moon diameter of 9550 pixels. This allows details as small as 1km across to be discerned! The superb quality of the image is shown by the detail below of Plato and the Alpine Valley. Craterlets are seen on the floor of Plato and the rille along the centre of the Alpine valley is clearly visible. The image quality is staggering! The team of Damian Peach, Pete lawrence, Dave Tyler, Bruce Kingsley, Nick Smith, Nick Howes, Trevor Little, David Mason, Mark and Lee Irvine with technical support from Ninian Boyle captured the video sequences from which 288 individual mozaic panes were produced. These were then stitched together to form the lunar image.

Plato and the Alpine Valley.

Please follow the link to the Lunar World Record website and it would be really great if you could donate to Sir Patrick Moore's chosen charity to either download a full resolution image or purchase a print.

The Planets

A montage of the Solar System. JPL / Nasa

Jupiter is now well placed in the late evening sky in the middle of an excellent apparition.

Jupiter

A Cassini image of Jupiter . Nasa

Jupiter. This month Jupiter, shining at magnitude -2.6, is visible for much of the night and dominates the southern sky in the evening. It was at opposition on the 5th January (when due south around midnight) so, at the start of the month is high in the sky during the evening - being at ~40 degrees elevation by 7 pm and rising to an elevation of over 60 degrees in the south at around 10 pm. This could not be better! By month's end Jupiter will be due south at ~8:30 pm. Jupiter is lying in the constellation Gemini moving westwards in retrograde motion towards the star Mebsuta - Epsilon Geminorum. With a small telescope you can observe the 4 Gallilean moons as they weave there way around it and, at times, be also able to pick out the Great Red Spot visible as an indentation of the South Equatorial belt.
See the highlights above.

Saturn

The planet Saturn. Cassini - Nasa

Saturn is now visible in the pre-dawn sky, rising at about 2 am at the start of February and at about 12:30 am at its end. Lying in Libra, it is shining with a magnitude of +0.4 and its disk has a diameter of ~17 arc seconds. The really good news is that the rings (with a diameter of 38 arc seconds) have now opened to around 23 degrees from the line of sight so presenting a magnificant view. With a small telescope one should be able to spot the Cassini Division that lies between the A and B rings and with a telescope of ~200 mm aperture the Enke Gap towards the edge of the A ring might be seen when the seeing is good. Sadly for those of us in the northern hemisphere, Saturn is now lying in the more southerly part of the ecliptic so, even at opposition, its elevation does not get that high. Even worse, this will not improve for many years to come.

Mars

A Hubble Space Telescope image of Mars.
Jim Bell et al. AURA / STScI / Nasa

Mars, lying in Virgo, rises around 11:30 the start of the month and about one hour earlier at month's end. Its magnitude increases from +0.2 to -0.5 during the month with its angular size increasing from 9 to 11 arc seconds. So, given good seeing, it is possible to see markings on its salmon-pink surface (~91% illumonated) such as the polar caps and Syrtis Major. The north polar region is tilted towards us by ~19 degrees so North Polar Cap should be particularly prominent. Mars is moving down across Virgo and, at the start of the month is just under 5 degrees to the upper left of Spica - Alpha Virginis. It ends the month 6 degrees to the left of Spica as it begins its westwards retrograde motion across the sky. See the highlight above.

Mercury

Messenger image of Mercury Nasa

Mercury reached its greatest elongation east (that is, furthest in angular separation over to the left of the Sun) of 18 degrees on January 31st when it lay about 10 degrees above the horizon 45 minutes after sunset lying near a slender crescent Moon. On February 1st, it will lie about 8 degrees below a slighly fuller crescent Moon. It magnitude will then be -0.6 and it will have an angular size of seven arc seconds and, given a low western horizon, will be visible for ~2 hours after sunset. Moving back towards the Sun in angle it will still remain visible for around an hour and a half after sunset by February 7th but by then its brightness will have dropped to magnitude +1. The angular size of its 20% illuminated disk then will have increased slightly to 8 arc seconds. Mercury then disappears from view passing in front of the Sun (inferior conjunction) on the 15th February but the reappearing in the pre dawn sky by month's end. Though then 22 degrees west of the Sun its elevation will be very low and, again at magnitude +1, will not be easy to spot.

See the highlight above.

Venus

Venus showing some cloud structure

Venus passed between the Earth and the Sun on the 11th of January so, in February, will be seen low above the eastern horizon before dawn. By mid February, the planet, shining at magnitude -4.6, will be visible 17 degrees above the south-eastern horison at sunrise. On Valentines Day it will show a 25% illuminated crescent disk some 41 arc seconds in diameter. As February draws to a close, Venus, remaining at magnitude -4.6, will present a fuller disk - rising to 36% - that will be 33 arc seconds across.

See the highlight above.

Radar image showing surface features

Find more planetary images and details about the Solar System: The Solar System

The Stars

The Mid Evening February Sky

The February Sky in the south - mid evening.

This map shows the constellations seen in the south during the evening. The brilliant constellation of Orion is seen in the south. Moving up and to the right - following the line of the three stars of Orion's belt - brings one to Taurus; the head of the bull being outlined by the V-shaped cluster called the Hyades with its eye delineated by the orange red star Aldebaran. Further up to the right lies the Pleaides Cluster. Towards the zenith from Taurus lies the constellation Auriga, whose brightest star Capella will be nearly overhead. To the upper left of Orion lie the heavenly twins, or Gemini, their heads indicated by the two bright stars Castor and Pollux. Down to the lower left of Orion lies the brightest star in the northern sky, Sirius, in the consteallation Canis Major. Up and to the left of Sirius is Procyon in Canis Minor. Rising in the East is the constellation of Leo, the Lion, with the planet Saturn up and to the right of Regulus its brightest star. Continuing in this direction towards Gemini is the faint constellation of Cancer with its open cluster Praesepe (also called the Beehive Cluster),the 44th object in Messier's catalogue. On a dark night it is a nice object to observe with binoculars. There is also information about the constellation Ursa Major,seen in the north, in the constellation details below.

The constellation Taurus

Taurus

Taurus is one of the most beautiful constellations and you can almost imagine the Bull charging down to the left towards Orion. His face is delineated by the "V" shaped cluster of stars called the Hyades, his eye is the red giant star Aldebaran and the tips of his horns are shown by the stars beta and zeta Tauri. Although alpha Tauri, Aldebaran, appears to lie amongst the stars of the Hyades cluster it is, in fact, less than half their distance lying 68 light years away from us. It is around 40 times the diameter of our Sun and 100 times as bright.

AAO Image of the Pleiades, M45, by David Malin

To the upper right of Taurus lies the open cluster, M45, the Pleiades. Often called the Seven Sisters, it is one of the brightest and closest open clusters. The Pleiades cluster lies at a distance of 400 light years and contains over 3000 stars. The cluster, which is about 13 light years across, is moving towards the star Betelgeuse in Orion. Surrounding the brightest stars are seen blue reflection nebulae caused by reflected light from many small carbon grains. These relfection nebulae look blue as the dust grains scatter blue light more efficiently than red. The grains form part of a molecular cloud through which the cluster is currently passing. (Or, to be more precise, did 400 years ago!)

VLT image of the Crab Nebula

Close to the tip of the left hand horn lies the Crab Nebula, also called M1 as it is the first entry of Charles Messier's catalogue of nebulous objects. Lying 6500 light years from the Sun, it is the remains of a giant star that was seen to explode as a supernova in the year 1056. It may just be glimpsed with binoculars on a very clear dark night and a telescope will show it as a misty blur of light.

Lord Rosse's drawing of M1

Its name "The Crab Nebula" was given to it by the Third Earl of Rosse who observed it with the 72 inch reflector at Birr Castle in County Offaly in central Ireland. As shown in the drawing above, it appeared to him rather lile a spider crab. The 72 inch was the world's largest telelescope for many years. At the heart of the Crab Nebula is a neutron star, the result of the collapse of the original star's core. Although only around 20 km in diameter it weighs more than our Sun and is spinning 30 times a second. Its rotating magnetic field generate beams of light and radio waves which sweep across the sky. As a result, a radio telescope will pick up very regular pulses of radiation and the object is thus also known a Pulsar. Its pulses are monitored each day at Jodrell Bank with a 13m radio telescope.

The constellation Orion

Orion

Orion, perhaps the most beautiful of constellations, will be seen in the south at around 11 - 12 pm during January. Orion is the hunter holding up a club and shield against the charge of Taurus, the Bull up and to his right. Alpha Orionis, or Betelgeuse, is a read supergiant star varying in size between three and four hundred times that of our Sun. The result is that its brightness varies somewhat. Beta Orionis, or Rigel, is a blue supergiant which, at around 1000 light years distance is about twice as far away as Betelgeuse. It has a 7th magnitude companion. The three stars of Orion's belt lie at a distance of around 1500 light years. Just below the lower left hand star lies a strip of nebulosity against which can be seen a pillar of dust in the shape of the chess-board knight. It is thus called the Horsehead Nebula. It shows up very well photographically but is exceedingly difficult to see visually - even with relativly large telescope.

The Horsehead Nebula: Anglo Australian Observatory

Beneath the central star of the belt lies Orion's sword containing one of the most beautiful sights in the heavens - The Orion Nebula. It is a region of star formation and the reddish colour seen in photographs comes from Hydrogen excited by ultraviolet emitted from the very hot young stars that make up the Trapesium which is at its heart. The nebula, cradling the trapesium stars, is a beautiful sight in binoculars or, better still, a telescope. To the eye it appears greenish, not red, as the eye is much more sensitive to the green light emitted by ionized oxygen than the reddish glow from the hydrogen atoms.

The Orion Nebula: David Malin

The constellation Ursa Major

Ursa Major

The stars of the Plough, shown linked by the thicker lines in the chart above, form one of the most recognised star patterns in the sky. Also called the Big Dipper, after the soup ladles used by farmer's wives in America to serve soup to the farm workers at lunchtime, it forms part of the Great Bear constellation - not quite so easy to make out! The stars Merak and Dubhe form the pointers which will lead you to the Pole Star, and hence find North. The stars Alcor and Mizar form a naked eye double which repays observation in a small telescope as Mizar is then shown to be an easily resolved double star. A fainter reddish star forms a triangle with Alcor and Mizar.
Ursa Major contains many interesting "deep sky" objects. The brightest, listed in Messier's Catalogue, are shown on the chart, but there are many fainter galaxies in the region too. In the upper right of the constellation are a pair of interacting galaxies M81 and M82 shown in the image below. M82 is undergoing a major burst of star formation and hence called a "starburst galaxy". They can be seen together using a low power eyepiece on a small telescope.

M81 and M82

Another, and very beautiful, galaxy is M101 which looks rather like a pinwheel firework, hence its other name the Pinwheel Galaxy. It was discovered in1781 and was a late entry to Messier's calalogue of nebulous objects. It is a type Sc spiral galaxy seen face on which is at a distance of about 24 million light years. Type Sc galaxies have a relativly small nucleus and open spiral arms. With an overall diameter of 170,000 light it is one of the largest spirals known (the Milky Way has a diameter of ~ 130,000 light years).

M101 - The Ursa Major Pinwheel Galaxy

Though just outside the constellation boundary, M51 lies close to Alkaid, the leftmost star of the Plough. Also called the Whirlpool Galaxy it is being deformed by the passage of the smaller galaxy on the left. This is now gravitationally captured by M51 and the two will eventually merge. M51 lies at a distance of about 37 million light years and was the first galaxy in which spiral arms were seen. It was discovered by Charles Messier in 1773 and the spiral structure was observed by Lord Rosse in 1845 using the 72" reflector at Birr Castle in Ireland - for many years the largest telescope in the world.

M51 - The Whirlpool Galaxy

Lying close to Merak is the planetary nebula M97 which is usually called the Owl Nebula due to its resemblance to an owl's face with two large eyes. It was first called this by Lord Rosse who drew it in 1848 - as shown in the image below right. Planetary nebulae ar the remnants of stars similar in size to our Sun. When all possible nuclear fusion processes are complete, the central core collpses down into a "white dwarf" star and the the outer parts of the star are blown off to form the surrounding nebula.

M97 - The Owl Planetary Nebula Lord Rosse's 1848 drawing of the Owl Nebula

Thursday 5 December 2013

The Night Sky in December c/o Ian Morison at the University of Manchester

The Night Sky December 2013

Compiled by Ian Morison

Image of the Month

Comet ISON: RIP

Comet ISON

Image: Damian Peach

ISON, the comet that few of us saw. I had hoped to show you how to look for what some had predicted would be the comet of the century during the early part of December. Sadly, as I write on the morning after ISON passed close behind the Sun on the 28th November, it looks as though Suns gravitational forces broke it up and little has emerged to give us a spectacular sight this December. This image, by the renowned Solar System imager Damian Peach, is by far the best of any taken as ISON approached the Sun, and I thank him for allowing me to reproduce it.
Postscript: December 3rd. Shown below is a composite image of the final hours of comet ISON as it rounded the Sun. As of December 2nd, it was just a cloud of debris no brighter than 8th magnitude. It is just possible that its remnants might be spotted in the pre dawn sky but it will be very hard to spot.

SOHO spacecraft final images of Comet ISON

To see more of Damian Peach's wonderful images of the solar system: Damian Peache's website

Highlights of the Month

December - the first good month to view Jupiter.

Jupiter imaged by Damian Peach

This is the first of several great months to observe Jupiter. It now lies Gemini and so is high in the ecliptic and hence, when due south, at an elevation of ~60 degrees. It is looking somewhat different than in the last few years as the north equatorial belt has become quite broad. The Great Red Spot is currently a pale shade of pink but can be easily seen as a large feature in the South Equatorial Belt.
The features seen in the Jovian atmosphere have been changing quite significantly over the last few years - for a while the South Equatorial Belt vanished completely (as seen in Damian's image) but has now returned to its normal wide state. The diagram on right shows the main Jovian features as imaged by the author at the beginning of December 2012.
The image by Damian Peach was taken with a 14 inch telescope in Barbados where the seeing can be particularly good. This image won the "Astronomy Photographer of the Year" competition in 2011. See more of Damian Peach's images: Damian Peaches Website"

Features in Jupiter's atmosphere - December 2013.

December 5th/6th - after sunset: Venus with a thin crescent Moon

Venus with a thin crescent Moon
Image: Stellarium/IM

About 45 minutes after sunset on the 5th and 6th and given a low horizon in the west-southwest one should be able to observe Venus over to the left of a thin crescent Moon.

Around the 1st to 6th December - Find M31, The Andromeda Galaxy - and perhaps M33 in Triangulum - with no Moon in the sky.

How to find M31
Image: Stellarium/IM

In the evening, the galaxy M31 in Andromeda is visible in the south-west. The chart provides two ways of finding it:
1) Find the square of Pegasus. Start at the top left star of the square - Alpha Andromedae - and move two stars to the left and up a bit. Then turn 90 degrees to the right, move up to one reasonably bright star and continue a similar distance in the same direction. You should easily spot M31 with binoculars and, if there is a dark sky, you can even see it with your unaided eye. The photons that are falling on your retina left Andromeda well over two million years ago!
2) You can also find M31 by following the "arrow" made by the three rightmost bright stars of Cassiopeia down to the lower right as shown on the chart.
Around new Moon (3rd December) you may also be able to spot M33, the third largest galaxy after M31 and our own galaxy in our Local Group of galaxies. It is a face on spiral and its surface brightness is pretty low so a dark, transparent sky will be needed to spot it using binoculars (8x40 or, preferably, 10x50). Follow the two stars back from M31 and continue in the same direction sweeping slowly as you go. It looks like a piece of tissue paper stuck on the sky just a bit brighter than the sky background. Good Hunting!

December 14th and 15th after midnight: the Geminid Meteor Shower.

Image:Stellarium/IM

The Geminids
The early mornings of December 14th and 15th will give us the chance, if clear, of observing the peak of the Geminid meteor shower. Sadly, this is not a good year, as a waxing Gibbous Moon high in Aries will hinder our view This means that you will only see the brighter trails by looking high up away from the glare of the Moon. An observing location well away from towns or cities will also pay dividends though. The relatively slow moving meteors arise from debris released from the asteroid 3200 Phaethon. This is unusual, as most meteor showers come from comets. The radiant - where the meteors appear to come from - is close to the bright star Castor in the constellation Gemini as shown on the chart. If it is clear it will be cold - so wrap up well, wear a woolly hat and have some hot drinks with you.

December 22nd/23rd - midnight onwards : the Ursid Meteor Shower

The Ursid meteor shower

The night of the 22nd/23rd December is when the Ursid meteor shower is at its best - though the peak rate of ~10-15 meteors per hour is not that great. The waning gibbous Moon lies in Leo - opposite in the sky - so moonlight will not greatly obstruct our view in the hours before dawn. The radiant lies close to the star Kochab in Ursa Minor (hence their name), so look northwards at a high elevation. Occasionally, there can be a far higher rate so its worth having a look should it be clear.

Around December 1st to 6th : Search for Neptune - with no Moon in the sky.

Neptune near closest approach
Image: Stellarium/IM

Neptune, with a magnitude of 7.8 should be easily seen in binoculars under a dark, early evening, sky. It will be due south around 18:30 in the evening. Neptune lies about 2 degrees above the star Iota Aquarii as shown on the chart. Iota Aquarii can be found by moving 5 degrees to the left and slightly upwards from the star Delta Capricorni.

December - 11th and 24th: The Alpine Valley

Alpine Valley region

An interesting valley on the Moon: The Alpine Valley
These are good nights to observe an interesting feature on the Moon if you have a small telescope. Close to the limb is the Appenine mountain chain that marks the edge of Mare Imbrium. Towards the upper end you should see the cleft across them called the Alpine valley. It is about 7 miles wide and 79 miles long. As shown in the image a thin rill runs along its length which is quite a challenge to observe. Over the next two nights following the 3rd/4th the dark crater Plato and the young crater Copernicus will come into view. This is a very interesting region of the Moon!

The Alpine valley and the crater Plato

M 109 imaged with the Faulkes Telescope

Messier galaxy M 109
Image: Danial Duggan
Faulkes Telescope North.

Spiral galaxy M109, imaged by Daniel Duggan.
This image was taken using the Faulkes Telescope North by Daniel Duggan - for some time a member of the Faulkes telescope team. M 109 is a Barred Spiral some 83 million light years away that lies is a loose collection of Galaxies called the Ursa Major Cloud that may contain over 50 galaxies.
Learn more about the Faulkes Telescopes and how schools can use them: Faulkes Telescope"

Observe the International Space Station

The International Space Station and Jules Verne passing behind the Lovell Telescope on April 1st 2008.
Image by Andrew Greenwood

The Moon

new moon	first quarter	full moon	last quarter
December 3rd	December 9th	December 17th	December 25th

Some Lunar Images by Ian Morison, Jodrell Bank Observatory: Lunar Images

A World Record Lunar Image

The 9 day old Moon.

Plato and the Alpine Valley.

The Planets

A montage of the Solar System. JPL / Nasa

Jupiter is now well placed in the late evening sky at the start of an excellent apparition.

Jupiter

A Cassini image of Jupiter . Nasa

Jupiter rises about 7:30 pm at the beginning of December and by late evening dominates the eastern sky. It transits (due South) at 3 am when it will be ~62 degrees above the horizon (in the UK)shining at magnitude -2.6 with a disk ~46 arc seconds across. Jupiter is lying in the constellation Gemini very close the the 3.5 magnitude star, Wasat - Delta Geminorum and, on the 10th, will lie just 15 arc minutes above Wasat. It is now moving in retrograde motion westwards across the sky. By month's end Jupiter will rise at 6 pm and transit at 2 am so will be high in the western sky as dawn breaks having a magnitude of -2.7 and a diameter of nearly 47 arc seconds. With a small telescope you can observe the 4 Gallilean moons as they weave there way around it and, at times, be also able to pick out the Great Red Spot visible as an indentation of the South Equatorial belt.
See the highlight above.

Saturn

The planet Saturn. Cassini - Nasa

Saturn. Having passed behind the Sun in early November Saturn is now visible in the pre-dawn sky, rising at about 5 am as December begins and at about 3:30 am at its end. It is shining with a magnitude of +0.6 and its disk has a diameter of ~15.5 arc seconds. The really good news is that the rings have now opened to around 21 degrees from the line of sight so present a magnificant view. Sadly for those of us in the northern hemisphere, Saturn is now lying in the more southerly part of the ecliptic so, even at opposition, its elevation does not get that high. Even worse, this will not improve for many years to come.

Mars

A Hubble Space Telescope image of Mars.
Jim Bell et al. AURA / STScI / Nasa

Mars, lying in Virgo, rises soon after midnight at the start of the month shining at magnitude +1.2. Its magnitude increases to +0.9 during the month with its angular size increasing from 5.6 to 6.8 arc seconds. So, given good seeing, it is possible to see markings on its salmon-pink surface such as the polar caps and Syrtis Major. So, we can say that Mar's apparition has really begun. Mars is moving down across Virgo and, at the very end of the month is very close to Porrima, Gamma Virginis.

Mercury

Messenger image of Mercury Nasa

Mercury is visible in the pre-dawn sky shining at magnitude +0.6 down to the lower left of Saturn as December begins. It brightens to -0.8 magnitudes during the first couple of weeks but, each morning. is a little lower above the horizon as dawn breaks and will be lost from view by mid December and passes behind the Sun (superior conjunction) on December 29th.

Venus

Venus showing some cloud structure

Venus shines at magnitude -4.9 in early December - a beacon in the western sky. However at this time of year the ecliptic is at quite a shallow angle to the horizon and, even worse, Venus, with a declination of -27, is very close to its furthest southern declination. The result is that it will lie close to the horizon in the south south-west and so, with an elevation of ~15 degrees above the horizon at sunset it will not be as prominent as one might expect. It is, however, very interesting to observe how its phase thins from 30 to 11% arc seconds during the first three weeks of the month whilst its angular size increases from 38 to 53 arc seconds. By month's end the phase has reduced to just 4% and it is almost one arc minute across. Venus pases in front of the Sun (inferior conjunction) on the 11th of next month.

See the highlight above.

Radar image showing surface features

Find more planetary images and details about the Solar System: The Solar System

The Stars

The Late Evening December Sky

The December Sky in the south - late evening

This maps shows the constellations seen towards the south in early and late evening. Setting towards the west in early evening is the beautiful region of the Milky Way containing both Cygnus and Lyra. Below is Aquilla. The three bright stars Deneb (in Cygnus), Vega (in Lyra) and Altair (in Aquila) make up the "Summer Triangle". East of Cygnus is the great square of Pegasus - adjacent to Andromeda in which lies M31, the Andromeda Nebula. To the north lies "w" shaped Cassiopeia and Perseus. The lower map shoesthe constellation Taurus, with its two lovely clusters, the Hyades and the Pleaides, and is also described in more detail below. as the evening draws on, Orion, the Hunter, follows Taurus into the eastern sky with the constellations Auriga, above, and Gemini, to the upper left. Later Sirius, in Canis Major will be seen to the lower left of Orion. Due to its brightness and scintillations caused by the atmosphere it often appears as a rainbow of colours flashing in the sky.

The constellations Pegasus and Andromeda

Pegasus and Andromeda

Pegasus
The Square of Pegasus is in the south during the evening and forms the body of the winged horse. The square is marked by 4 stars of 2nd and 3rd magnitude, with the top left hand one actually forming part of the constellation Andromeda. The sides of the square are almost 15 degrees across, about the width of a clentched fist, but it contains few stars visibe to the naked eye. If you can see 5 then you know that the sky is both dark and transparent! Three stars drop down to the right of the bottom right hand corner of the square marked by Alpha Pegasi, Markab. A brighter star Epsilon Pegasi is then a little up to the right, at 2nd magnitude the brightest star in this part of the sky. A little further up and to the right is the Globular Cluster M15. It is just too faint to be seen with the naked eye, but binoculars show it clearly as a fuzzy patch of light just to the right of a 6th magnitude star.
Andromeda
The stars of Andromeda arc up and to the left of the top left star of the square, Sirra or Alpha Andromedae. The most dramatic object in this constellation is M31, the Andromeda Nebula. It is a great spiral galaxy, similar to, but somewhat larger than, our galaxy and lies about 2.5 million light years from us. It can be seen with the naked eye as a faint elliptical glow as long as the sky is reasonably clear and dark. Move up and to the left two stars from Sirra, these are Pi amd Mu Andromedae. Then move your view through a rightangle to the right of Mu by about one field of view of a pair of binoculars and you should be able to see it easily. M31 contains about twice as many stars as our own galaxy, the Milky Way, and together they are the two largest members of our own Local Group of about 3 dozen galaxies.

M31 - The Andromeda Nebula

M33 in Triangulum
If, using something like 8 by 40 binoculars, you have seen M31 as described above, it might well be worth searching for M33 in Triangulum. Triangulum is
the small faint constellation just below Andromeda. Start on M31, drop down to Mu Andromedae and keep on going in the same direction by the same distance as you have moved from M31 to Mu Andromedae. Under excellent seeing conditions (ie., very dark and clear skies) you should be able to see what looks like a little piece of tissue paper stuck on the sky or a faint cloud. It appears to have uniform brightness and shows no structure. The shape is irregular in outline - by no means oval in shape and covers an area about twice the size of the Moon. It is said that it is just visible to the unaided eye, so it the most distant object in the Universe that the eye can see. The distance is now thought to be 3.0 Million light years - just greater than that of M31.

M33 in triangulum - David Malin

The constellation Taurus

Taurus

The Hyiades and Pleiades. Copyright: Alson Wong.

More beautiful images by Alson Wong : Astrophotography by Alson Wong
To the upper right of Taurus lies the open cluster, M45, the Pleiades. Often called the Seven Sisters, it is one of the brightest and closest open clusters. The Pleiades cluster lies at a distance of 400 light years and contains over 3000 stars. The cluster, which is about 13 light years across, is moving towards the star Betelgeuse in Orion. Surrounding the brightest stars are seen blue reflection nebulae caused by reflected light from many small carbon grains. These relfection nebulae look blue as the dust grains scatter blue light more efficiently than red. The grains form part of a molecular cloud through which the cluster is currently passing. (Or, to be more precise, did 400 years ago!)

VLT image of the Crab Nebula

Lord Rosse's drawing of M1

The constellation Orion

Orion

The Horsehead Nebula: Anglo Australian Observatory

The Orion Nebula: David Malin