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November 14 Observing Guide
- Neill
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10 years 1 month ago #102219
by Neill
November 14 Observing Guide was created by Neill
OBSERVING GUIDE
(Please note all times are UT and are based on the location of Belfast and covers November)
The Sun
At the start of the month, the Sun rises at 07:30 and sets at 16:50. By month's end, it rises at 08:20 and sets at 16:05.
The Planets
Mercury is at greatest western elongation on the 1st and is well placed for observation in the morning sky in the first half of the month. This will be its best morning appearance during the year. At the start of the month, it rises at 05:30 and is mag -0.5.
Venus is not visible this month.
Mars is visible low in the evening sky and is in Sagittarius this month. At the start of the month, it sets at 19:15 and by month's end at 19:20. It fades from mag +0.9 to mag +1.0 during the month.
Jupiter is at western quadrature on the 14th and becomes visible in the evening sky by month's end. It is in Leo this month. At the start of the month, it rises at 23:40 and by month's end, it rises at 22:00. It brightens from mag -2.1 to mag -2.2 during the month.
Saturn is at conjunction on the 18th and is not visible this month.
Uranus is visible in Pisces this month. It rises during daylight hours during the month and sets at 03:00 by month's end. It fades from mag +5.7 to mag +5.8 and lies to the S of Kaht (Epsilon (ε) Piscium, mag +4.3) and Linteum (Delta (δ) Piscium, mag +4.4) during the month.
Neptune is at eastern quadrature on the 27th and is visible in Aquarius this month. It rises during daylight hours during the month and sets at 23:10 by month's end. It maintains its brightness at mag +7.9 during the month and lies near to Sigma (σ) Aquarii, mag +4.8 during the month.
The Moon
The full moon is on the 6th with the last quarter moon on the 14th. The new moon is on the 22nd with the first quarter moon on the 29th.
On the evening of the 1st, the waxing gibbous moon lies 5° to the NW of Neptune at around 20:00.
On the evening of the 4th, the waxing gibbous moon lies 2° to the NE of Uranus at around 20:00.
On the evening of the 7th, the waning gibbous moon lies SW of M45 - The Pleiades and NW of Aldebaran (Alpha (α) Tauri, mag +0.9) at around 20:00. On the following evening the moon lies 1° to the NE of the star at around the same time.
On the night of the 12th/13th, the waning gibbous moon lies 8° to the W of M44 - The Beehive Cluster at around midnight.
On the mornings of the 14th and 15th, the moon lies near to Jupiter. On the 14th, the waning gibbous moon lies 8° to the W of it and on the 15th; the waning crescent moon lies to the S of it. On the 15th, the moon also lies 6° to the W of Regulus (Alpha (α) Leonis, mag +1.4). On both mornings, look at around 01:00.
On the morning of the 19th, the waning crescent moon lies to the N of Spica (Alpha (α) Virginis, mag +1.0) at around 06:00.
On the evening of the 26th, the waxing crescent moon lies to the N of Mars at around 18:00.
On the evening of the 28th, the waxing crescent moon lies to the W of Neptune at around 18:00.
Meteors
The best time to observe meteor showers is when the moon is below the horizon; otherwise its bright glare limits the number you will see especially the fainter ones. Below is a guide to this month's showers.
The Taurids have 2 peaks, firstly on the evening of the 5th and then on the evening of the 12th with a ZHR of 5 for each peak. The radiant on both nights is visible from 20:00. The Southern peak is on the 5th, but a waxing gibbous moon in Pisces will spoil the show. The Northern peak on the 12th fares a little better with a waning gibbous moon in Cancer rising at 21:40. This allows for around 90 minutes viewing time without lunar interference.
The Leonids peak on the evening of the 17th/18th with a ZHR of 15. The radiant is visible from 01:00 on the morning of the 18th. This allows for around 2 hours of viewing time without lunar interference before a waning crescent moon rises at 03:00 in Virgo. They are typically very fast meteors with a speed of around 71 km/s compared with the Perseids at 59 km/s and the Geminids at 35 km/s.
There are additional minor showers this month, details of which can be found at meteorshowersonline.com/calendar.html or www.imo.net/calendar/2014
Asteroids
Asteroid (6) Hebe is at opposition on the morning of the 17th at mag +7.4. It is visible in Eridanus from 22:00 through to 04:00 on the night of the 16th/17th.
Finder charts and further information about other fainter asteroids can be found at; britastro.org/computing/charts_asteroid.html in the source list below.
Comets
There are no bright comets visible during the month.
Finder charts and further information about other fainter comets can be found at www.aerith.net , cometchasing.skyhound.com , www.ast.cam.ac.uk/%7Ejds/ , in-the-sky.org , kometen.fg-vds.de/fgk_hpe.htm, www.nightskyhunter.com/index.html and www.rasnz.org.nz in the source list below. Any above estimates for predicting a comet's brightness/status are based on current information at the time of writing the guide and the comet may be brighter/dimmer than the above predictions or may no longer be intact to observe.
Deep Sky
On the deep sky front this month, galaxies M81 and M82 can be observed in Ursa Major. In Andromeda, M31 - The Andromeda galaxy can be observed along with its satellite galaxies M32 and M110. In Perseus, there is the open cluster M34 and the excellent Double Cluster - NGC 869 and 884. In Triangulum, there is the galaxy M33. In Auriga there are three open clusters M36, M37 and M38 and also M35 in Gemini. Taurus has the excellent Pleiades - M45, the Hyades and also M1 - The Crab Nebula. Orion returns to our skies with M42 - The Great Orion Nebula and also Cancer with M44 - The Beehive Cluster.
General Notes
Always keep an eye out for Aurorae. The Zodiacal Light can be seen in the West after evening twilight has disappeared or in the East before the morning twilight. The best time of year to see the phenomenon is late-Feb to early-April in the evening sky and September/October in the morning sky - it's then that the ecliptic, along which the cone of the zodiacal light lies, is steepest in our skies. The Gegenschein can be seen in the area of the sky opposite the sun. To view either, you must get yourself to a very dark site to cut out the light pollution. When trying to observe either of these phenomena, it is best to do so when the moon is below the horizon. A new appendix has been added explaining some of the more technical terms used in the guide.
Clear Skies
Neill McKeown
Information Sources Used and Links
www.skyviewcafe.com ; Sky at Night Magazine Observing Guide and CD; www.aerith.net ; cometchasing.skyhound.com ; www.ast.cam.ac.uk/%7Ejds/ ; kometen.fg-vds.de/fgk_hpe.htm ; www.rasnz.org.nz ; Stardust Magazine; britastro.org/computing/charts_asteroid.html ; in-the-sky.org ; www.nightskyhunter.com/index.html www.eagleseye.me.uk/Sky/Wordpress/;http:...meris/ephemeris.html ; eco.mtk.nao.ac.jp/cgi-bin/koyomi/cande/phenomena_en.cgi ;
Philip's Stargazing 2014; Patrick Moore's 2014 Yearbook of Astronomy; www.heavens-above.com ; www.spaceweather.com ;meteorshowersonline.com/calendar.html ; www.timeanddate.com/astronomy/ ; www.imo.net/calendar/2014 - International Meteor Organisation; messier.seds.org/ - The Messier Catalogue website; www.seds.org/messier/xtra/ngc/ngc.html - NGC Catalogue website; www.irishastronomy.org - Irish Federation of Astronomy Societies Website; irishastro.org.uk/- Irish Astronomical Association website; www.eaas.co.uk - Northern Ireland Amateur Astronomy Society;
Appendix
The ZHR or Zenithal Hourly Rate is the number of meteors an observer would see in one hour under a clear, dark sky with a limiting apparent magnitude of 6.5 and if the radiant of the shower were in the zenith. The rate that can effectively be seen is nearly always lower and decreases as the radiant is closer to the horizon. The Zenith is the overhead point in the sky.
The radiant is the point in the sky, from which (to a planetary observer) meteors appear to originate, i.e. the Perseids, for example, are meteors which appear to come from a point within the constellation of Perseus. When the radiant is quoted as "circumpolar", it is never below the horizon and visible all night, otherwise the times quoted are when the constellation in which the radiant lies rises above the horizon in the East.
A fireball is defined by the International Astronomical Union as a meteor brighter than any of the planets, i.e. magnitude -4 or brighter. The International Meteor Organisation alternatively defines it as a meteor which would have a magnitude of -3 or brighter at the zenith.
The ° symbol in the guide is that for degrees. A degree is two full moon widths to give an idea for judging any distances quoted in the guide. There are 60 arcminutes in a degree.
An asterism is a collection of stars seen in Earth's sky which form simple patterns which are easy to identify, i.e. the Big Dipper. They can be formed from stars within the same constellation or by stars from more than one constellation. Like the constellations, they are a line of sight phenomenon and the stars whilst visible in the same general direction, are not physically related and are often at significantly different distances from Earth.
Mag is short for magnitude which is the measure of an object's brightness. The smaller the number, the brighter the object. The brightest object in the sky is the Sun at mag -26, the full moon is mag -12 and Venus the brightest planet is mag -4. The brightest stars are mag -1. If there is a 1 mag difference between two objects - there is a difference in brightness of a factor of 2.5 between the two objects. For example the full moon is eight magnitudes brighter than Venus on average which means it is 1,526 times brighter than Venus. Objects down to mag +6 can be seen with the naked eye under very dark skies.
Local time is always quoted in the guide and this means for November - February - universal time (UT)/GMT is used and for April to September - daylight savings time (DST, = GMT+1). For the months of March and October when the clocks go forward/back respectively, both times will be used and attention should be paid to any times at the end of these months for that change.
Deep Sky Objects such as galaxies, nebulae and star clusters are classified in catalogues such as the Messier catalogue for objects like M44 - M for Messier. Another example of a catalogue would the New General catalogue whose objects have the prefix NGC. There are links for websites to both catalogues in the section above.
Perihelion is the point in the orbit of a planet, asteroid or comet where it is at the nearest point in its orbit to the sun. It is the opposite of Aphelion, which is when the object is at the farthest point in its orbit from the sun. For the earth, the comparative terms used are perigee and apogee and for the moon, pericynthion and apocynthion are sometimes used.
The Planets
From Earth - Mercury and Venus are the inner planets in the solar system and Mars, Jupiter, Saturn, Uranus and Neptune are the outer planets. Below is a short guide as to how both the inner and outer planets move around the sun. The above pictorial guide should hopefully help in this.
The Inner Planets
These are best seen when at Greatest Eastern/Western elongation and are not visible when at either Inferior/Superior conjunction. Greatest Eastern elongation is when the inner planet is at its furthest point east from the sun as seen from Earth and visible in the evening sky in the West after sunset, Western elongation is when it's at its furthest point west from the sun as seen from Earth and visible in the morning sky in the East before sunset. Inferior conjunction occurs when the inner planet is between the Sun and the Earth. Superior conjunction occurs when the inner planet is on the other side of the Sun as seen from Earth.
From our Northerly latitudes, the ecliptic, along which the planets move, lies at a very shallow angle to the horizon after sunset in the autumn and before sunrise in the spring. This means that any of the planets will be difficult to see when fairly close to the Sun in the evening sky in the autumn or in the morning sky in the spring. In particular, Mercury is more or less invisible from here when at Eastern elongation in the autumn or at Western elongation in the spring, because it lies so close to the horizon and is never above the horizon except in daylight or bright twilight.
The normal cycle for an inner planet is Superior Conjunction - Greatest Eastern Elongation - Inferior Conjunction - Greatest Western Elongation - Superior Conjunction. After superior conjunction, the planet moves away from the Sun as seen from Earth and becomes visible in the evening sky after a period of time. It then moves past the point of Greatest Eastern Elongation and moves back towards the Sun as seen from Earth until a point when it is not visible and at Inferior Conjunction. After this the planet appears in the morning sky for a time, before again slipping into the Sun's glare as seen from Earth. The duration of this cycle will depend on the planet's closeness to the Sun, i.e. Mercury completes the above cycle in around 4 months.
The Outer Planets
These are best seen when at opposition and are not visible when at conjunction. Opposition occurs when the earth is between the sun and the outer planet. It is the best time to observe them because the planet is visible all through the night and it is due South and at its highest at about midnight. The planet is also at its closest point in its orbit to Earth - making it appear brighter. Conjunction occurs when the outer planet is on the other side of the Sun as seen from Earth.
If the planet is at or near it furthest point South along the ecliptic, then it won't get very high in the sky even at opposition - just as the Sun never gets high in the sky in midwinter. This happens when opposition occurs near midsummer when the planet is opposite the Sun in the sky and in midsummer the Sun is high, so the planet will be low. The opposite of course applies in winter.
The normal cycle for an outer planet is Conjunction - Western Quadrature - Opposition - Eastern Quadrature - Conjunction. After conjunction, the planet moves away from the Sun as seen from Earth and becomes visible again. The planet from this point on rises earlier and earlier in the morning sky and eventually becomes visible in the evening sky. At Western Quadrature it is at its highest at sunrise and by opposition it is in the same position by midnight. By Eastern Quadrature, it is past its best and is at its highest at sunset, meaning it is rising in daytime and setting earlier and earlier until a point when it sets too close to the Sun as seen from Earth and is no longer visible. The duration of this cycle will depend on the planet's closeness to the Sun, i.e. Jupiter completes the above cycle in around 13-14 months.
(Please note all times are UT and are based on the location of Belfast and covers November)
The Sun
At the start of the month, the Sun rises at 07:30 and sets at 16:50. By month's end, it rises at 08:20 and sets at 16:05.
The Planets
Mercury is at greatest western elongation on the 1st and is well placed for observation in the morning sky in the first half of the month. This will be its best morning appearance during the year. At the start of the month, it rises at 05:30 and is mag -0.5.
Venus is not visible this month.
Mars is visible low in the evening sky and is in Sagittarius this month. At the start of the month, it sets at 19:15 and by month's end at 19:20. It fades from mag +0.9 to mag +1.0 during the month.
Jupiter is at western quadrature on the 14th and becomes visible in the evening sky by month's end. It is in Leo this month. At the start of the month, it rises at 23:40 and by month's end, it rises at 22:00. It brightens from mag -2.1 to mag -2.2 during the month.
Saturn is at conjunction on the 18th and is not visible this month.
Uranus is visible in Pisces this month. It rises during daylight hours during the month and sets at 03:00 by month's end. It fades from mag +5.7 to mag +5.8 and lies to the S of Kaht (Epsilon (ε) Piscium, mag +4.3) and Linteum (Delta (δ) Piscium, mag +4.4) during the month.
Neptune is at eastern quadrature on the 27th and is visible in Aquarius this month. It rises during daylight hours during the month and sets at 23:10 by month's end. It maintains its brightness at mag +7.9 during the month and lies near to Sigma (σ) Aquarii, mag +4.8 during the month.
The Moon
The full moon is on the 6th with the last quarter moon on the 14th. The new moon is on the 22nd with the first quarter moon on the 29th.
On the evening of the 1st, the waxing gibbous moon lies 5° to the NW of Neptune at around 20:00.
On the evening of the 4th, the waxing gibbous moon lies 2° to the NE of Uranus at around 20:00.
On the evening of the 7th, the waning gibbous moon lies SW of M45 - The Pleiades and NW of Aldebaran (Alpha (α) Tauri, mag +0.9) at around 20:00. On the following evening the moon lies 1° to the NE of the star at around the same time.
On the night of the 12th/13th, the waning gibbous moon lies 8° to the W of M44 - The Beehive Cluster at around midnight.
On the mornings of the 14th and 15th, the moon lies near to Jupiter. On the 14th, the waning gibbous moon lies 8° to the W of it and on the 15th; the waning crescent moon lies to the S of it. On the 15th, the moon also lies 6° to the W of Regulus (Alpha (α) Leonis, mag +1.4). On both mornings, look at around 01:00.
On the morning of the 19th, the waning crescent moon lies to the N of Spica (Alpha (α) Virginis, mag +1.0) at around 06:00.
On the evening of the 26th, the waxing crescent moon lies to the N of Mars at around 18:00.
On the evening of the 28th, the waxing crescent moon lies to the W of Neptune at around 18:00.
Meteors
The best time to observe meteor showers is when the moon is below the horizon; otherwise its bright glare limits the number you will see especially the fainter ones. Below is a guide to this month's showers.
The Taurids have 2 peaks, firstly on the evening of the 5th and then on the evening of the 12th with a ZHR of 5 for each peak. The radiant on both nights is visible from 20:00. The Southern peak is on the 5th, but a waxing gibbous moon in Pisces will spoil the show. The Northern peak on the 12th fares a little better with a waning gibbous moon in Cancer rising at 21:40. This allows for around 90 minutes viewing time without lunar interference.
The Leonids peak on the evening of the 17th/18th with a ZHR of 15. The radiant is visible from 01:00 on the morning of the 18th. This allows for around 2 hours of viewing time without lunar interference before a waning crescent moon rises at 03:00 in Virgo. They are typically very fast meteors with a speed of around 71 km/s compared with the Perseids at 59 km/s and the Geminids at 35 km/s.
There are additional minor showers this month, details of which can be found at meteorshowersonline.com/calendar.html or www.imo.net/calendar/2014
Asteroids
Asteroid (6) Hebe is at opposition on the morning of the 17th at mag +7.4. It is visible in Eridanus from 22:00 through to 04:00 on the night of the 16th/17th.
Finder charts and further information about other fainter asteroids can be found at; britastro.org/computing/charts_asteroid.html in the source list below.
Comets
There are no bright comets visible during the month.
Finder charts and further information about other fainter comets can be found at www.aerith.net , cometchasing.skyhound.com , www.ast.cam.ac.uk/%7Ejds/ , in-the-sky.org , kometen.fg-vds.de/fgk_hpe.htm, www.nightskyhunter.com/index.html and www.rasnz.org.nz in the source list below. Any above estimates for predicting a comet's brightness/status are based on current information at the time of writing the guide and the comet may be brighter/dimmer than the above predictions or may no longer be intact to observe.
Deep Sky
On the deep sky front this month, galaxies M81 and M82 can be observed in Ursa Major. In Andromeda, M31 - The Andromeda galaxy can be observed along with its satellite galaxies M32 and M110. In Perseus, there is the open cluster M34 and the excellent Double Cluster - NGC 869 and 884. In Triangulum, there is the galaxy M33. In Auriga there are three open clusters M36, M37 and M38 and also M35 in Gemini. Taurus has the excellent Pleiades - M45, the Hyades and also M1 - The Crab Nebula. Orion returns to our skies with M42 - The Great Orion Nebula and also Cancer with M44 - The Beehive Cluster.
General Notes
Always keep an eye out for Aurorae. The Zodiacal Light can be seen in the West after evening twilight has disappeared or in the East before the morning twilight. The best time of year to see the phenomenon is late-Feb to early-April in the evening sky and September/October in the morning sky - it's then that the ecliptic, along which the cone of the zodiacal light lies, is steepest in our skies. The Gegenschein can be seen in the area of the sky opposite the sun. To view either, you must get yourself to a very dark site to cut out the light pollution. When trying to observe either of these phenomena, it is best to do so when the moon is below the horizon. A new appendix has been added explaining some of the more technical terms used in the guide.
Clear Skies
Neill McKeown
Information Sources Used and Links
www.skyviewcafe.com ; Sky at Night Magazine Observing Guide and CD; www.aerith.net ; cometchasing.skyhound.com ; www.ast.cam.ac.uk/%7Ejds/ ; kometen.fg-vds.de/fgk_hpe.htm ; www.rasnz.org.nz ; Stardust Magazine; britastro.org/computing/charts_asteroid.html ; in-the-sky.org ; www.nightskyhunter.com/index.html www.eagleseye.me.uk/Sky/Wordpress/;http:...meris/ephemeris.html ; eco.mtk.nao.ac.jp/cgi-bin/koyomi/cande/phenomena_en.cgi ;
Philip's Stargazing 2014; Patrick Moore's 2014 Yearbook of Astronomy; www.heavens-above.com ; www.spaceweather.com ;meteorshowersonline.com/calendar.html ; www.timeanddate.com/astronomy/ ; www.imo.net/calendar/2014 - International Meteor Organisation; messier.seds.org/ - The Messier Catalogue website; www.seds.org/messier/xtra/ngc/ngc.html - NGC Catalogue website; www.irishastronomy.org - Irish Federation of Astronomy Societies Website; irishastro.org.uk/- Irish Astronomical Association website; www.eaas.co.uk - Northern Ireland Amateur Astronomy Society;
Appendix
The ZHR or Zenithal Hourly Rate is the number of meteors an observer would see in one hour under a clear, dark sky with a limiting apparent magnitude of 6.5 and if the radiant of the shower were in the zenith. The rate that can effectively be seen is nearly always lower and decreases as the radiant is closer to the horizon. The Zenith is the overhead point in the sky.
The radiant is the point in the sky, from which (to a planetary observer) meteors appear to originate, i.e. the Perseids, for example, are meteors which appear to come from a point within the constellation of Perseus. When the radiant is quoted as "circumpolar", it is never below the horizon and visible all night, otherwise the times quoted are when the constellation in which the radiant lies rises above the horizon in the East.
A fireball is defined by the International Astronomical Union as a meteor brighter than any of the planets, i.e. magnitude -4 or brighter. The International Meteor Organisation alternatively defines it as a meteor which would have a magnitude of -3 or brighter at the zenith.
The ° symbol in the guide is that for degrees. A degree is two full moon widths to give an idea for judging any distances quoted in the guide. There are 60 arcminutes in a degree.
An asterism is a collection of stars seen in Earth's sky which form simple patterns which are easy to identify, i.e. the Big Dipper. They can be formed from stars within the same constellation or by stars from more than one constellation. Like the constellations, they are a line of sight phenomenon and the stars whilst visible in the same general direction, are not physically related and are often at significantly different distances from Earth.
Mag is short for magnitude which is the measure of an object's brightness. The smaller the number, the brighter the object. The brightest object in the sky is the Sun at mag -26, the full moon is mag -12 and Venus the brightest planet is mag -4. The brightest stars are mag -1. If there is a 1 mag difference between two objects - there is a difference in brightness of a factor of 2.5 between the two objects. For example the full moon is eight magnitudes brighter than Venus on average which means it is 1,526 times brighter than Venus. Objects down to mag +6 can be seen with the naked eye under very dark skies.
Local time is always quoted in the guide and this means for November - February - universal time (UT)/GMT is used and for April to September - daylight savings time (DST, = GMT+1). For the months of March and October when the clocks go forward/back respectively, both times will be used and attention should be paid to any times at the end of these months for that change.
Deep Sky Objects such as galaxies, nebulae and star clusters are classified in catalogues such as the Messier catalogue for objects like M44 - M for Messier. Another example of a catalogue would the New General catalogue whose objects have the prefix NGC. There are links for websites to both catalogues in the section above.
Perihelion is the point in the orbit of a planet, asteroid or comet where it is at the nearest point in its orbit to the sun. It is the opposite of Aphelion, which is when the object is at the farthest point in its orbit from the sun. For the earth, the comparative terms used are perigee and apogee and for the moon, pericynthion and apocynthion are sometimes used.
The Planets
From Earth - Mercury and Venus are the inner planets in the solar system and Mars, Jupiter, Saturn, Uranus and Neptune are the outer planets. Below is a short guide as to how both the inner and outer planets move around the sun. The above pictorial guide should hopefully help in this.
The Inner Planets
These are best seen when at Greatest Eastern/Western elongation and are not visible when at either Inferior/Superior conjunction. Greatest Eastern elongation is when the inner planet is at its furthest point east from the sun as seen from Earth and visible in the evening sky in the West after sunset, Western elongation is when it's at its furthest point west from the sun as seen from Earth and visible in the morning sky in the East before sunset. Inferior conjunction occurs when the inner planet is between the Sun and the Earth. Superior conjunction occurs when the inner planet is on the other side of the Sun as seen from Earth.
From our Northerly latitudes, the ecliptic, along which the planets move, lies at a very shallow angle to the horizon after sunset in the autumn and before sunrise in the spring. This means that any of the planets will be difficult to see when fairly close to the Sun in the evening sky in the autumn or in the morning sky in the spring. In particular, Mercury is more or less invisible from here when at Eastern elongation in the autumn or at Western elongation in the spring, because it lies so close to the horizon and is never above the horizon except in daylight or bright twilight.
The normal cycle for an inner planet is Superior Conjunction - Greatest Eastern Elongation - Inferior Conjunction - Greatest Western Elongation - Superior Conjunction. After superior conjunction, the planet moves away from the Sun as seen from Earth and becomes visible in the evening sky after a period of time. It then moves past the point of Greatest Eastern Elongation and moves back towards the Sun as seen from Earth until a point when it is not visible and at Inferior Conjunction. After this the planet appears in the morning sky for a time, before again slipping into the Sun's glare as seen from Earth. The duration of this cycle will depend on the planet's closeness to the Sun, i.e. Mercury completes the above cycle in around 4 months.
The Outer Planets
These are best seen when at opposition and are not visible when at conjunction. Opposition occurs when the earth is between the sun and the outer planet. It is the best time to observe them because the planet is visible all through the night and it is due South and at its highest at about midnight. The planet is also at its closest point in its orbit to Earth - making it appear brighter. Conjunction occurs when the outer planet is on the other side of the Sun as seen from Earth.
If the planet is at or near it furthest point South along the ecliptic, then it won't get very high in the sky even at opposition - just as the Sun never gets high in the sky in midwinter. This happens when opposition occurs near midsummer when the planet is opposite the Sun in the sky and in midsummer the Sun is high, so the planet will be low. The opposite of course applies in winter.
The normal cycle for an outer planet is Conjunction - Western Quadrature - Opposition - Eastern Quadrature - Conjunction. After conjunction, the planet moves away from the Sun as seen from Earth and becomes visible again. The planet from this point on rises earlier and earlier in the morning sky and eventually becomes visible in the evening sky. At Western Quadrature it is at its highest at sunrise and by opposition it is in the same position by midnight. By Eastern Quadrature, it is past its best and is at its highest at sunset, meaning it is rising in daytime and setting earlier and earlier until a point when it sets too close to the Sun as seen from Earth and is no longer visible. The duration of this cycle will depend on the planet's closeness to the Sun, i.e. Jupiter completes the above cycle in around 13-14 months.
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