March 2016 Sky Guide PDF Print E-mail

This page is dedicated to the practical observer including :

 

OBSERVING GUIDE

(Please note all times are UT unless otherwise stated and are based on an observing location of Belfast and covers the month of March)

The Sun

At the start of the month, the Sun rises at 07:15 and sets at 18:00. By month's end, it rises at 07:00 ST and sets at 20:00 ST. Summer Time begins at 01:00 on the morning of the 27th with the clocks going forward one hour.

 

The Planets

Mercury is at superior conjunction on the 23rd and is not visible this month.

Venus is not visible this month.

Mars is visible in the morning sky this month, moving from Libra to Scorpius. At the start of the month, it rises at 01:25 and by month's end at 01:20 ST. It brightens from mag +0.3 to mag -0.4 during the month.

Jupiter is at opposition on the 8th and is visible in the evening sky in Leo this month. At the start of the month, it rises at 18:35 and by month's end; it is visible as soon as darkness falls. It maintains its brightness at mag -2.3 during the month.

Saturn is at western quadrature on the 6th and is visible in the morning sky and is in Ophiuchus this month. At the start of the month, it rises at 02:55 and by month's end at 02:00 ST. It brightens from mag +1.2 to mag +1.1 during the month.

Uranus is visible in Pisces at the start of the month when it sets at 21:25, but is gone from view by mid-month. It lies to the S of Epsilon (ε) Piscium, mag +4.3.

Neptune is not visible this month.

 

The Moon

The last quarter moon is on the 1st with the new moon on the 9th. The first quarter moon is on the 15th with the full moon on the 23rd. There is a 2nd last quarter moon on the 31st.

On the morning of the 1st, the waning gibbous moon lies 5° to the E of Mars at around 03:00.

On the morning of the 2nd, the waning crescent moon lies 6° to the N of Saturn at around 04:00.

On the evening of the 10th, the waxing crescent moon lies to the S of Uranus at around 19:00.

On the evening of the 14th, the waxing crescent moon lies 3° to the NE of Aldebaran (Alpha (α) Tauri, mag +0.9) at around 20:00.

On the evening of the 20th, the waxing gibbous moon lies 7° to the S of Regulus (Alpha (α) Leonis, mag +1.4) at around 20:00.

On the evening of the 21st, the waxing gibbous moon lies 5° to the W of Jupiter at around 20:00.

On the evening of the 24th, the waning gibbous moon lies to the N of Spica (Alpha (α) Virginis, mag +1.0) at around 22:00.

On the mornings of the 29th and 30th, the waning gibbous moon lies close to Saturn. On the 29th, it lies to the NW of the planet. On the same morning, it also lies 5° to the NE of Mars. On the 30th, it lies 8° to the E of the ringed planet.

 

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.

There are no bright meteor showers this month.

There may be additional minor showers this month, details of which can be found at meteorshowersonline.com/calendar.html or http://imo.net/files/data/calendar/cal2016.pdf

 

Asteroids

Asteroid (10) Hygiea is opposition on the evening of the 15th at mag +9.4. It is visible in Leo from 19:00 on the evening of the 15th.

Asteroid (6) Hebe is at opposition on the morning of the 17th at mag +9.8. It is visible in Coma Berencies from 20:00 on the evening of the 16th.

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

Comet C/2013 US10 Catalina is visible in the evening sky this month. Current estimates have it at mag +8 and it will fade during March. It is circumpolar and moves from Camelopardalis into Perseus during the month. At the start of the month, it lies to the S of NGC 1502, a mag +6.9 open cluster at the edge of Kemble's Cascade. On the evening of the 23rd, it lies close to NGC 1528, a mag +6.4 open cluster and then on the evening of the 28th, it lies close to NGC 1545, a mag +6.4 open cluster.

Comet C/2014 S2 (PanSTARRS) is currently mag +10 and is expected to remain at similar brightness for the month ahead. It starts the month in Ursa Minoris, then moves into Draco by mid-month and then into Ursa Major by month's end. It will be circumpolar and lies close to Pherkad (Gamma (γ) Ursa Minoris, mag +3.1) at the start of the month.

Finder charts and further information about the above and other fainter comets can be found at www.aerith.net, cometchasing.skyhound.com, www.ast.cam.ac.uk/%7Ejds/ , in-the-sky.org, www.nightskyhunter.com/index.html in the source list below. Any of the above estimates are based on current information at the time of writing the guide and can be wrong - "Comets are like cats; they have tails, and they do precisely what they want", David H Levy.

 

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 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. In Orion we have M42 - The Great Orion Nebula and also Cancer with M44 - The Beehive Cluster and M67. Check out the constellation Canes Venatici with the globular cluster - M3 and several galaxies including M51 - the Whirlpool Galaxy and M63 - the Sunflower Galaxy. In Leo, we have several galaxies on view including The Leo Triplet - M65, M66 and NGC 3628. M95, M96 and M105 can also be observed in Leo. The place to really find galaxies is in Virgo. The Virgo Super Cluster can be found here with numerous galaxies on view. Also in Virgo, M104 - the Sombrero Galaxy can be found. In Coma Berenices, there is M64 - the Black-Eye Galaxy.

 

General Notes

Always keep an eye out for Aurorae. The Spring or Vernal Equinox is on March 20th which sees the end of winter and the beginning of spring. Other interesting naked eye phenomena to look out for include the Zodiacal Light and the Gegenschein.

Both are caused by sunlight reflecting off dust particles which are present in the solar system. 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

www.skyviewcafe.com ; Sky at Night Magazine Observing Guide and CD;
www.aerith.net ; http://cometchasing.skyhound.com ;
www.ast.cam.ac.uk/%7Ejds/;
http://kometen.fg-vds.de/fgk_hpe.htm ;
www.rasnz.org.nz ;
Stardust Magazine;
http://britastro.org/computing/charts_asteroid.html ;
http://in-the-sky.org ;
http://www.nightskyhunter.com/index.html
http://www.eagleseye.me.uk/Sky/Wordpress/;
http://astropixels.com/ephemeris/ephemeris.html;
http://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/;
http://www.imo.net/calendar/2014 - International Meteor Organisation;
http://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;
http://irishastro.org.uk/- Irish Astronomical Association website;
www.niaas.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.


 

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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 its 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.


 

ISS Passes

For detailed sightings information and sky charts, check out Heavens Above or Calsky .

Iridium Flares

Every night there are a number of Iridium flares of varying brightness, some can be up to Mag-8 which are very impressive to watch. Check out Heavens Above or Calsky for the latest predictions.

Welcome to the Forum of the Northern Ireland Amateur Astronomy Society, whether you've come just to browse or wish to join in.
You'll find a wealth of information both here and on our website at www.niaas.co.uk, and we welcome any questions about buying a telescope, observing, or any other astronomy-based matters.

Enjoy your stay.

Philip Matchett
NIAAS Webmaster
 

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