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The Night Sky November 2013

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

NGC 7027

Planetary Nebula NGC7027

Image: Hubble Legacy Archive, NASA, ESA - Processing: Delio Tolivia Cadrecha

NGC 7027 is one of the brightest planetary nebula in the sky, first discovered in 1878.   Lying in the constellation Cygnus, it only appears as an indistinct spot in amateur telescopes and is rarely viewed.   It is believed that its progenitor star exploded about 600 years ago and the dust and gas contained within it is about three times the mass of our Sun.

Highlights of the Month

November 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 6th and given a low horizon in the west-southwest one should be able to observe Venus a little below and to the left of a thin crescent Moon.

November 5/6th and 12/13th early morning: Shadow transits of Io and Europa across the face of Jupiter

Shadow transits on Jupiter

Given a small telescope and clear skies, these mornings give one a chance of observing the shadows of Io and Europa as they cross the face of Jupiter.   The shadow transits start at 23:00 on the evening of the 5th as the shadow of Io falls upon the surface of Jupiter.   Just after midnight, Io will begin to pass across the face of Jupiter and at 00:49 Io and its shadow will be joined by Europa's shadow.   In turn, Europa will begin to pass in front of Jupiter at 02:46.   On the morning of the 13th Io's shadow will begin to fall on Jupter at 01:04 and Io will begin to pass in front of Jupiter at 02:04.   Europa's shadow will begin to fall on the surface at 03:15 and it will begin to pass in front of Jupiter at 05:53.   The free program "WinJUPOS" is an excellent resource with which to predict such events.

Around the 3rd November - Find M31 - The Andromeda Galaxy - and perhaps M33 in Triangulum

How to find M31
Image: Stellarium/IM

In the evening, the galaxy M31 in Andromeda is visible in the south 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 November) 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!

November 16th/17th - late evening : The Leonid Meteor Shower

Leonid meteor
A Leonid crossing the Sword of Orion

Every year, on the nights of November 16th and 17th, the Earth passed close to the trails of cometry debris from Comet Temple-Tuttle which produce the annual Leonid Meteor shower.  The wonderful image shows one of the 2001 Leonids burning up in the atmosphere as it crossed the constellation of Orion.  Sadly, this year, the meteor shower occurs at the time of full Moon, so its light will only allow the brightest of the fast moving meteors to be observed.   The best time to observe them will be after midnight as our hemisphere is facing the stream of cometary debris.   The dust particles that are swept up by the Earth are released as Comet Temple-Tuttle rounds the Sun every 33 years.   As implied by the name, the radiant of the shower - from where the meteors appear to radiate from - lies within the head or Sickle of the constellation Leo the Lion.

November 1st to 7th: With no Moon, a good time 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.   Neptune lies close to the star Iota Aquarii which can be found by moving 5 degrees to the left and slightly upwards from the star Delta Capricorni.   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.

November - Comet ISON should become visible in binoculars or a telescope in the hour before dawn - perhaps best seen from the 16th onwards.

Comet ISON
Track of Comet ISON
Image: Stellarium/IM

As November begins, comet ISON lies below Mars in the pre-dawn sky and may well be picked up with a telescope.   As it brightens in the latter half of the month it should be possible to spot comet ISON with binoculars as its brightness was predicted to reach magnitude 3-4.   However, recently it has not been brightening as much as predicted so may well not be so bright and,sadly, this might mean that ISON will not be the spectacular comet that many had hoped for.   As it nears the Sun it is moving rapidly across the sky - from Leo across Virgo and Libra into Scorpius.   On the 17th and 18th it will lie close to Spica in Virgo.   Around the 21st it closes on Mercury and Saturn and will lie below them from the 24th onwards, but by this time it will probably be lost in the Sun' glare.   It passes very close to the Sun on the 28th and its ~3km diameter nucleus may well be split into many small pieces.   How this will affect its visibility durign December is hard to predict - we will just have to keep our fingers crossed!   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 November and December and 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".

November 26th - before dawn: a close conjunction of Mercury and Saturn.

Saturn and Mercury
A close conjunction of Mercury and Saturn
Image: Stellarium/IM

About 40 minutes before sunrise on the 26th, if clear and given a low eastern horizon, you should be able to spot Saturn (at magnitude +0.6) just above Mercury, three times brighter at magnitude -0.7.   at 01:00 that morning they will have been just 1/3rd of a degree apart but their seperation will have increased to 0.4 degrees as they come above the horizon.   Comet ISON may be visible below them just above the horizon.

Learn the Mare on the Moon.

Mare on the Moon
Mare on the Moon
Image:Ian Morison

Why not use the annotated image of the full Moon to learn the locations of the Moon's Mare.  You can see some of them with your unaided eye and binoculars will enable you to spot them all.

NGC 891 imaged with the Faulkes Telescope

NGC 891
Edge-on galaxy NGC 891
Image: Danial Duggan
Faulkes Telescope North.

Galaxy NGC 891, 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.   NGC 891 is an edge-on spiral lying in the constellation Andromeda at a distance of 27 million light years.   We think that this is very much as our own galaxy might look when seen edge-on.

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
November 3rd November 10th November 17th November 25th

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 we will also be able to observe Comet ISON as it nears the Sun.


A Cassini image of Jupiter . Nasa

Jupiter rises about 9 pm at the beginning of November and transits at 5 am when it will be ~60 degrees above the horizon in the south shining at magnitude -2.4 with a disk ~41 arc seconds across.   Jupiter is lying in the constellation Gemini very close the the 3.5 magnitude star, Wasat - Delta Geminorum.   On November 7th it begins its retrograde motion westwards across the sky.   By month's end Jupiter will rise at 7pm and transit at 3 am so will be high in the southern sky as dawn breaks having a magnitude of -2.6 and a diameter of nearly 45 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.   Nicely, both equatorial bands are showing well at the present time.   Shadow transits of Io and Europa take place on the 5th/6th - beginning at 23:00 on the 5th - and 12/13th of November - beginning at 03:00.

See the highlight above.


The planet Saturn. Cassini - Nasa

Saturn,is at conjunction behind the Sun on the 6th of November so will only become visible in the pre-dawn sky towards the end of the month.   On the 22nd November it might be seen along with Mercury and comet ISON low above the eastern horizon.   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 at about 01:30 at the start of the month shining at magnitude +1.5.   It will be easily visible with binoculars in the pre-dawn sky - but please cease using them at sunrise!   Its magnitude increases to +1.2 during the month with its angular size increasing from 4.9 to 5.6 arc seconds.   It is now above the angular size of 5 arc seconds when, given good seeing, it is possible to see markings on its salmon-pink surface.   So, we can say that Mar's apparition has really begun.   Mars moves from Leo into Virgo on the 25th.


Messenger image of Mercury Nasa

Mercury passes throught inferior conjunction (between the Earth and the Sun) on the first of the month and will become visible in the pre-dawn sky from about November 9th shining at magnitude +0.8.   It brightens to -0.7 magnitude by the 20th and remains well visible until early December in what is its best morning apparition of 2013.

See the highlight above.


Venus showing some cloud structure

Venus reaches its greatest elongation from the Sun on November the 1st and this is usually when it is best seen.   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.   On the 6th, Venus will be farther south than at any time since 1930.   The result is that it will lie close to the horizon in the south south-west and so, even with an elevation above the horizon at sunset increasing from 9 to 14 degrees and its magnitude increasing from -4.5 to -4.8 during the month, will not be as prominent as one might expect.

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 November Sky

November Sky
The November Sky in the south - early evening

This map shows the constellations seen towards the south in early 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 and Perseus. The constellation Taurus, with its two lovely clusters, the Hyades and Pleiades is rising in the east during the late evening.

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 Albireo (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 Albireo, 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

The constellation 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.

The Hyades and Pleiades
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!)

The Crab Nebula
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.

The Crab Nebula
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.