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The Night Sky October 2013

Compiled by Ian Morison

Note: We are sorry that there were problems accessing this “Night Sky” page in mid September and these same problems have made it difficult to prepare the web page for this month.   We apologise for any anomalies that might be found and will aim to rectify them as soon as possible.

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

RS Puppis

Cepheid Variable, RS Puppis

Image: Hubble Legacy Archive, NASA, ESA - Processing: Stephen Byrne

The pulsating star RS Puppis, seen in the image centre, is some ten times more massive than our Sun and on average 15,000 times more luminous.   RS Pup is a Cepheid variable star, a class of stars whose brightness is used to estimate distances to nearby galaxies as one of the first steps in establishing the cosmic distance scale.   As RS Pup pulsates over a period of about 40 days, its regular changes in brightness are also seen within the nebula, but delayed in time the further away from the central star.   By using measurements of the time delay and angular size of the nebula, has allowed astronomers to geometrically determine the distance to RS Pup to be 6,500 light-years, with a remarkably small error of plus or minus 90 light-years.   This has allowed the absolute brightness of RS Pup to be accurately determined and, by extension, that of other Cepheid Variable stars.   This, in turn, has allowed the distances to galaxies beyond the Milky Way to be found more accurately.

Highlights of the Month

October 8th - after sunset: Venus, Saturn and Mercury along with a thin crescent Moon

Venus, Saturn, Mercury and a crescent Moon
Image: Stellarium/IM

About 45 minutes after sunset on the 8th and given a low horizon in the west-southwest it might be possible to observe three planets and a thin crescent Moon.   Venus will lie below the Moon with Saturn over to the right just above Mercury.   One will need a very low western horizon and Mercury is only just above the horizon as the Sun has set.

October 14th – before dawn: Mars just above Regulus in Leo.

Mars above Regulus in Leo
Image: Stellarium/IM

Just before dawn on the mornings of the 14th, Mars will be seen passing just above Regulus in Leo.   Mars will be shining at magnitude +1.4 with Regulus at +1.6.   There will be a very nice colour contrast between the two; Mars pink-red and Regulus blue-white.   Note: Comet ISON will be above Mars on this morning – see the plot for the positions of the comet below.   Mars and comet ISON track each other across the sky during this month, being particularly close from the 15th to the 19th.

Early October - Find the globular cluster in Hercules and spot the "Double-double" in Lyra

Use binoculars to find M13 and the Double-double.
Image: Stellarium/IM

There are two very nice objects to spot with binoculars in the southern sky after dark this month.   Two thirds of the way up the right hand side of the 4 stars that make up the "keystone" in the constellation Hercules is M13, the best globular cluster visible in the northern sky.   Just to the left of the bright star Vega in Lyra is the multiple star system Epsilon Lyrae often called the double-double.   With binoculars a binary star is seen but, when observed with a telescope, each of these two stars is revealed to be a double star - hence the name!   More details can be found within the "Astronomical A-List" (Link is at upper left.)

October - Use a telescope to view two of the best planetary nebula in the northern sky - The Ring and Dumbbell Nebulae in Lyra and Vulpecular respectivly.

Use a telescope to observe two bright planetary nebulae
Image: Stellarium/IM

When it gets dark during October the beautiful region of the sky including Cygnus, Lyra and Aquilla will be high in the south.   The constellations brightest stars: Vega in Lyra, Deneb in Cygnus and Altair in Aquila making up what is called the summer triangle.   Within this region lie two of the brightest planetary nebulae that we can observe in the northern skies.   Between Beta and Gamma Lyrae, the pair of bright stars lying below Vega, is the Ring Nebula, M57, seen as a tiny "smoke ring" in a small telescope whilst, below Cygnus in Vulpecula is the Dumbbell Nebula, M27.   M27 can even be seen with 10 x 50 binoculars given a dark, transparent, sky.   Details of both these beautiful objects can be found within the "Astronomical A List" section of our website (link at upper left) or within the author's book "Pocket Guide to Stars and Galaxies" for which the list was initially produced.

October – Still a good month to observe Neptune with a small telescope.

Neptune in Aquarius
Image: Stellarium/IM

Neptune came into opposition - when it is nearest the Earth - on the 27th of August, so will be seen in the evening this month.   Its magnitude is +7.9 so Neptune is easily spotted in binoculars lying in the constellation Aquarius as shown on the chart.   It rises to an elevation of ~27 degrees when due south.   Given a telescope of 8 inches or greater aperture and a dark tranparent night it should even be possible to spot its moon Triton.

October - Comet ISON should become visible in a medium sized telescope and will just above Regulus in Leo on the 16th and close to Mars between the 16th and 19th of the month.

Comet ISON
Comet ISON in Leo
Image: Stellarium/IM

Before dawn towards the end of the month and given a 6" or greater telescope, it may be possible to spot comet ISON whose brightness was predicted to increase from magnitude 10 to magnitude 7 during October.   However, recently it has not been brightening as much as predicted and, when observed on August 12th, had a magnitude of 14.3 rather than its predicted magnitude of between 12.3 and 13.5.   Sadly, this might mean that ISON will not be the spectacular comet that many had hoped for.   On the 16th, it will pass just above Regulus in Leo and stays within one degree of the planet Mars from the 16th to the 19th of October.   This page will try to keep you updated as the weeks progress.   The app "SkySafari Plus" for ipad and android devices will download the comets orbital elements and show its position in the sky during the next few months.   This app has been used to plot its position during the month.   An excellent website relating to the comet can be found by searching for “waiting for ison”.

October 26th: Mons Piton and Cassini

Location of Mons Piton:IM

Mons Piton and the crater Cassini
Best seen just before Third Quarter, Mons Piton is an isolated lunar mountain located in the eastern part of Mare Imbrium, south-east of the crater Plato and west of the crater Cassini.   It has a diameter of 25 km and a height of 2.3 km.   Its height was determined by the length of the shadow it casts.  Cassini is a 57km crater that has been flooded with lava.   The crater floor has then been impacted many times and holds within its borders two significant craters, Cassini A, the larger and Cassini B.

Mons Piton
Mons Piton and Cassini

A Messier Object imaged with the Faulkes Telescope: M57 in Lyra

Ring Nebula, M57
The Ring Nebula, M57
Image:Danial Duggan
Faulkes Telescope North.

Planetary Nebula M82, 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.   Lying at at distance of 2.3 thousand light years in the constellation Lyra, it is the remnant of a star like our Sun.   The core of the star has contracted down to an object about the size of the Earth supported by electron degeneracy pressure and is seen in the centre of the object.   The outer parts of the star were blasted out into space forming the "ring" (or torus) that we see.   Though showing very well in images, the central "star", called a "White Dwarf" is hard to see visually.

Learn more about the Faulkes Telescopes and how schools can use them: Faulkes Telescope"

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 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

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 moon first quarter full moon last quarter
October 4th October 11th October 18th October 26th

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

A World Record Lunar Image

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
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
A montage of the Solar System. JPL / Nasa

Jupiter is now well placed in the pre-dawn sky at the start of an excellent apparition. Hopefully, by October’s end, a chance to observe comet ISON as well given a small telescope or binoculars.


A Cassini image of Jupiter . Nasa

Jupiter rises about midnight BST at the beginning of October and about 2 hours earlier by its end.   At the start of astronomical twilight, it will be ~40 degrees above the horizon in the south-east shining at magnitude -2.2 with a disk ~38 arc seconds across.   Jupiter is lying in the constellation Gemini and on October 4th it passes just above the Star Delta Geminorum (Wasat) shining at magnitude 3.5 – a magnitude brighter than Jupiter’s brightest moon, Ganymeade.   On October 12th, Jupiter is 90 degrees to the right of the Sun as seen from Earth and this is an excellent time for viewing eclipse and shadow transits of the four Gallilean moons as they weave their way around it.   By month's end Jupiter will be high in the southern sky before dawn breaks having a magnitude of -2.4 and a diameter of 41 arc seconds.   With a small telescope one should, at times, be also able to pick out the Great Red Spot visible as an indentation of the South Equatorial belt.   Nicely, both equatorial bands are showing well at the present time.


The planet Saturn. Cassini - Nasa

Saturn, lying in Libra, may just be visible low above the horizon for the first couple of weeks of October lying well to the right of Venus in the west.   Binoculars may well be needed to pick it out in the twilight sky when it will have a magnitude of +0.7 and an angular size of 15.5 arc seconds.   The rings have opened out to ~17 degrees from the line of sight and we are now observing the planet's southern hemisphere whilst much of the northern hemisphere will be hidden by the rings.   As this month it can only be seen at a very low elevation, telescopic views will not be good but, with a small scope, it may just be possible to spot Saturn's largest moon, Titan.   Saturn is now lying in the more southerly part of the ecliptic so, even at opposition, its elevation does not get that high when seen from our northern latitudes.   Sadly, this will get worse for quite a number of years to come.

See the highlight above.


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

Mars, lying in Leo, rises some 4 to 5 hours before the Sun this month shining at magnitude +1.6.   It will be easily visible with binoculars in the pre-dawn sky - but please cease using them at sunrise!   Its magnitude of +1.6 remains constant during the month with its angular size increasing from 4.4 to 4.9 arc seconds.   It is then very close to an angular size of 5 arc seconds when, given good seeing, it is possible to see markings on its salmon-pink surface.   So, by the end of the month, we could say that Mar’s apparition has really begun.   It lies very close to Regulus, Alpha Leonis, on the morning of the 12th and its pink-red colour should make a very nice colour contrast with the blue-white of Regulus – shining a little brighter at magnitude 1.4.   Mars lies very close to comet ISON from October 16th to the 19th.

See the highlights above.


Messenger image of Mercury Nasa

Mercury might just be seen very low above the horizon about half an hour after sunset down to the lower right of Saturn.   Even though, at magnitude -0.1 as October begins, it is twice as bright as Saturn it will still be hard to see when using binoculars or a telescope.   Its angular size increases from 6 to 10 arc seconds during the month but, to be honest, there is not much to be gained from observing it.   On the 7th October it might be glimpsed 5 degrees below Saturn with, above Saturn, a slender crescent Moon.

See the highlights above.


Venus showing some cloud structure

Venus can be seen above the horizon in the west-southwest after sunset as its brightness increases from -4.2 to -4.5 magnitudes during the month.   It is moving quickly across the heavens; initially in Libra, it passes through Scopius (above Antares) and Ophiuchus before reaching Sagittarius on November 1st when it is at its furthest angular separation form the Sun.   Its angular size increases during the month from 18 to 25 arc seconds as the percentage of the disk that is illuminated decreases from 73 to 50%.   It is an interesting fact that during its long apparition its brightness hardly changes as when it is further away from Earth more of its smaller disk is illuminated by the Sun with, for example, 50% of a 25 arc second disk equivalent in apparent reflecting area to 73% of an 18 arc second disk.

See the highlight above.

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