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The Night Sky October 2008

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


Active Region 1002
Image: SOHO consortium, EIT, ESA, NASA

At the present time the Sun is in a transitional period between two solar cycles - the ~11 period during which the solar activity (and hence no of sunspots) rises fairly quickly over a period of ~ 4 years and then falls more slowly. But the start of the next solar cycle is now somewhat overdue and this low level of activity has not been seen for several decades. In addition the Ulysses spacecraft which has been monitoring the strength of the solar wind - another measure of solar activity - observes a 50 year low. It could be that the next solar cycle is, at last, beginning as an active region, shown upper right, has recently appeared complete with sunspots. This may hereld the start of a new solar cycle with an increasing number of sunspots predicted to appear intil solar maximum around 2012. It will be very interesting to observe what happens over the next few months!

Highlights of the Month

October 26th: Mercury, Saturn and a waning crescent Moon

Mercury, Satrun and the crescent Moon
Pre-dawn Sky on 26th October
Image: Stellarium/IM

Mercury reaches greatest eastern elongation from the Sun on the 22nd October and so presents the best chance of observing it in the pre-dawn sky this year about 90 minutes before dawn. Saturn rises before Mercury and so will be seen higher in the sky to its upper right below the constellation Leo with its bright star Regulus. On 26th October They will be joined by a waning crescent Moon.

October: Try and spot Vesta, the brightest of the minor planets

Path of Vesta through the head of Cetus the Whald
Image: Stellarium/IM

Vesta is the second most massive object in the asteroid belt after Ceres( now termed a dwarf planet) but it is the brightest. In the early morning hours of October, when Taurus the Bull in high in the eastern sky, it may be found crossing the head of Cetus the whale. This can be found as a circle of stars below the Pleiades Cluster in Taurus, and "pointed to" by the "V" shaped Hyades cluster. At magnitude +6.5, you will need binoculars to spot it and a good method to be sure that you have seen it is the sketch out the positions of the stars in the region and look again a few days later to see which starlike object has moved.

Below is a plot that you could "left click" on to give the full size image, then "right click" on that and "save picture as" to enable you to print out a template on which you could plot the position of Vesta.

Head of Cetus
The Head of Cetus the Whale
Image: Easysky/IM

Find M31 - The Andromeda Galaxy

How to find M31
Image: Stellarium/IM

In the late evening, the galaxy M31 in Andromeda is visible in the south-east. The chart above provided 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 resonably bright star and continue a similar distance again 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. Good Hunting!

Around October 21st: the Orionid Meteor Shower

October 21st - around 1- 2 am
Image: Stellarium/im

Though the Orionids are not one of the most spectaculer showers with peak rates around 20 per hour, they are interesting as it is believed that the meteors originate from Comet Halley. It is worth looking out for them for a week around the 21st as the shower is long lived. They will best be seen in the hours before dawn when Orion is high in the southern sky. The star chart shows where they appear to radiate from - called the radiant - at the upper left of Orion, close to the boarder with Gemini. Its best to look almost vertically where the sky is most transparent. Sadly,the Moon will be close to the radiant this year so one will only see the very brightest. The Halley meteors are amongst the fastest and enter the upper atmosphere at ~41 km per hour and often leave what are called persistant trains - streaks of ionized gas as the incoming dust particles burn up in the atmosphere. Halley's Comet actually gives us two meteor showers per year as we intersect its orbit twice as the Earth orbits the Sun. The other is in May and the shower is called the Eta Aquarid shower.

Seek out Uranus with binoculars or a telescope

This month: Uranus near to Phi Aquarii.
Image: Stellarium/IM

October is another good month to observe the planet Uranus - perhaps for the first time - with binoculars, a small telescope or even your unaided eye! &nb &nbs Uranus, with a magnitude of 5.8, lies ~ 2 degrees up and to the left of the 4th magnitude star Phi Aquarii. (If Phi Aquarii is the centre of a clock, Uranus is at 10:00) During the month it drifts slowly westward and is very close to the star 96 Aquarii which has a very similar magnitde of 5.4 magnitide. Binoculars will easily show it and a small telescope will show a blue-green disc just under 4 arc seconds in angular diameter. Around the time of new moon (at the very beginning and end of the month) under dark and transparent skies you even be able to see it with your unaided eyes. Have a go!

Observe the International Space Station

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 in the last week or so of July 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

3rd Quarter 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 first quarter full moon last quarter
October 28th October 7th October 14th October 21st

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

The Planets

 A montage of the Solar System
A montage of the Solar System. JPL / Nasa


A Cassini image of Jupiter . Nasa

Jupiter is seen low down in the south-west as nightfall begins. It lies above the "teapot" in Sagittarius. It begins October with an angular size of 39.3 arc seconds which slowly reduces to 37 arc seconds as the month progresses. In like manner, its brightness reduces from -2.3 to -2.2 magnitudes during the month.

Jupiter is now at the lowest point of the ecliptic in the sky and will only rise to about 10 degrees elevation above the horizon after nightfall. Thus, sadly, this year our views of Jupiter from northern latitudes have been rather poor. Despite the low elevation, even a small telescope will show the Galilean Moons as they weave their way around it. Due to refraction, we see Jupiter at very slightly different elevations in the different colours of the spectrum, thus bluring the image. A cleaner image may seen if one observes through a narrow band filter such as a green filter or, even better, if you have an 8" scope or above with a filter like an OIII filter only letting a very narrow band of light through.


The planet Saturn. Cassini - Nasa

Saturn is now visible in the pre-dawn sky and is seen higher as the month progresses. It will be best seen at the end of the month at ~05:00 UT. when it reaches an elevation of ~25 degrees before the Sun rises. It has a magnitude of ~+1 throughout the month. This is significantly less than it often appears as the rings will then be at an angle of just 4 degrees from edge on! As we move towards into next year, this angle will reduce until the rings are edge on and become invisible to us. Saturn is close to the thin crescent Moon on the 25th and 26th of October. See highlight above.


Messinger image of Mercury Nasa

Mercury: passes between us and the Sun on the 6th of October, but soon re-appears in the pre-dawn sky to be seen again in the latter half of the month. It reaches western elongation (when it is furthest from the Sun) on 22nd of the month lying in the constellation Virgo.

See highlight above


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

Mars lies so close to the Sun this month that it cannot be observed.


Venus showing some cloud structure

Venus can be seen very low in the west after sunset shining at magnitude -3.8 so it is possible to spot it without the use of binoculars. It is gradually moving further in angle from the Sun so will remain in the evening sky for longer after the Sun has set as the month progresses whilst its brightness increases fractionally to a magnitude of -4. It starts October with an angular size of 12.2 arc seconds and its disk is 92% illuminated. By the end of the month, the angular size has increased to 13.3 arc seconds but the percentage illuminated will have dropped. These two effects tend to cancel out in the way they affect its apparent brightness which is why the brightness remains almost constant.

Radar Image of Venus
Radar image showing surface features

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

The Stars

The Evening October Sky

October Sky
The October Sky in the south - mid evening

This map shows the constellations seen towards the south in mid evening. To the south in early evening - moving over to the west as the night progresses 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 with Perseus below.

The constellations Lyra and Cygnus

Cygnus and Lyra
Lyra and Cygnus

This month the constellations Lyra and Cygnus are seen almost overhead as darkness falls with their bright stars Vega, in Lyra, and Deneb, in Cygnus, making up the "summer triangle" of bright stars with Altair in the constellation Aquila below. (see sky chart above)


Lyra is dominated by its brightest star Vega, the fifth brightest star in the sky. It is a blue-white star having a magnitude of 0.03, and lies 26 light years away. It weighs three times more than the Sun and is about 50 times brighter. It is thus burning up its nuclear fuel at a greater rate than the Sun and so will shine for a correspondingly shorter time. Vega is much younger than the Sun, perhaps only a few hundred million years old, and is surrounded by a cold,dark disc of dust in which an embryonic solar system is being formed!

There is a lovely double star called Epsilon Lyrae up and to the left of Vega. A pair of binoculars will show them up easily - you might even see them both with your unaided eye. In fact a telescope, provided the atmosphere is calm, shows that each of the two stars that you can see is a double star as well so it is called the double double!

The Double Double
Epsilon Lyra - The Double Double

Between Beta and Gamma Lyra lies a beautiful object called the Ring Nebula. It is the 57th object in the Messier Catalogue and so is also called M57. Such objects are called planetary nebulae as in a telescope they show a disc, rather like a planet. But in fact they are the remnants of stars, similar to our Sun, that have come to the end of their life and have blown off a shell of dust and gas around them. The Ring Nebula looks like a greenish smoke ring in a small telescope, but is not as impressive as it is shown in photographs in which you can also see the faint central "white dwarf" star which is the core of the original star which has collapsed down to about the size of the Earth. Still very hot this shines with a blue-white colour, but is cooling down and will eventually become dark and invisible - a "black dwarf"! Do click on the image below to see the large version - its wonderful!

M57 - The Ring Nebula
M57 - the Ring Nebula
Image: Hubble Space telescope

M56 is an 8th magnitude Globular Cluster visible in binoculars roughly half way between Alberio (the head of the Swan) and Gamma Lyrae. It is 33,000 light years away and has a diameter of about 60 light years. It was first seen by Charles Messier in 1779 and became the 56th entry into his catalogue.

M56 - Globular Cluster
M56 - Globular Cluster


Cygnus, the Swan, is sometimes called the "Northern Cross" as it has a distinctive cross shape, but we normally think of it as a flying Swan. Deneb,the arabic word for "tail", is a 1.3 magnitude star which marks the tail of the swan. It is nearly 2000 light years away and appears so bright only because it gives out around 80,000 times as much light as our Sun. In fact if Deneb where as close as the brightest star in the northern sky, Sirius, it would appear as brilliant as the half moon and the sky would never be really dark when it was above the horizon!

The star, Albireo, which marks the head of the Swan is much fainter, but a beautiful sight in a small telescope. This shows that Albireo is made of two stars, amber and blue-green, which provide a wonderful colour contrast. With magnitudes 3.1 and 5.1 they are regarded as the most beautiful double star that can be seen in the sky.

Alberio: Diagram showing the colours and relative brightnesses

Cygnus lies along the line of the Milky Way, the disk of our own Galaxy, and provides a wealth of stars and clusters to observe. Just to the left of the line joining Deneb and Sadr, the star at the centre of the outstretched wings, you may, under very clear dark skys, see a region which is darker than the surroundings. This is called the Cygnus Rift and is caused by the obscuration of light from distant stars by a lane of dust in our local spiral arm. the dust comes from elements such as carbon which have been built up in stars and ejected into space in explosions that give rise to objects such as the planetary nebula M57 described above.

There is a beautiful region of nebulosity up and to the left of Deneb which is visible with binoculars in a very dark and clear sky. Photographs show an outline that looks like North America - hence its name the North America Nebula. Just to its right is a less bright region that looks like a Pelican, with a long beak and dark eye, so not surprisingly this is called the Pelican Nebula. The photograph below shows them well.

The North American Nebula
The North American Nebula

Brocchi's Cluster An easy object to spot with binoculars in Gygnus is "Brocchi's Cluster", often called "The Coathanger",although it appears upside down in the sky! Follow down the neck of the swan to the star Alberio, then sweep down and to its lower left. You should easily spot it against the dark dust lane behind.

The Coathanger
Brocchi's Cluster - The Coathanger

The constellations Pegasus and Andromeda

Pegasus and Andromeda
Pegasus and Andromeda


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.


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.

M 31 - The Andromeda Nebula
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