Categotry Archives: Education


Massive storm pulls ices from Saturn’s depth

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Cassini spacecraft images show the development of the largest storm seen on the planet since 1990. On Saturn, not only are storms much bigger than on Earth, they’re far more violent, with vertical winds of more than 300 miles per hour.

Massive storm pulls ices from Saturn’s depth

Cassini spacecraft images show the development of the largest storm seen on the planet since 1990. On Saturn, not only are storms much bigger than on Earth, they’re far more violent, with vertical winds of more than 300 miles per hour.

Once every 30 years or so, or roughly one Saturnian year, a monster storm rips across the northern hemisphere of the ringed planet.

Image credit: NASA/JPL-Caltech/Space Science Institute

This series of images from NASA’s Cassini spacecraft shows the development of the largest storm seen on the planet since 1990. These true-color and composite near-true-color views chronicle the storm from its start in late 2010 through mid-2011, showing how the distinct head of the storm quickly grew large but eventually became engulfed by the storm’s tail. Image credit: NASA/JPL-Caltech/Space Science Institute

In 2010, the most recent and only the sixth giant storm on Saturn observed by humans began stirring. It quickly grew to superstorm proportions, reaching 15,000 kilometers (more than 9,300 miles) in width and visible to amateur astronomers on Earth as a great white spot dancing across the surface of the planet.

Now, thanks to near-infrared spectral measurements taken by NASA’s Cassini orbiter and analysis of near-infrared color signatures by researchers at UW-Madison, Saturn’s superstorm is helping scientists flesh out a picture of the composition of the planet’s atmosphere at depths typically obscured by a thick high-altitude haze.

The key finding: cloud particles at the top of the great storm are composed of a mix of three substances: water ice, ammonia ice, and an uncertain third constituent that is possibly ammonium hydrosulfide. According to the Wisconsin researchers, the observations are consistent with clouds of different chemical compositions existing side-by-side, although a more likely scenario is that the individual cloud particles are composed of two or all three of the materials.

Writing in the current edition (Sept. 9, 2013) of the journal Icarus, a team led by UW-Madison Space Science and Engineering Center planetary scientists Lawrence Sromovsky, and including Kevin Baines and Patrick Fry, reports the discovery of the icy forms of water and ammonia. Water in the form of ice has never before been observed on Saturn.

“We think this huge thunderstorm is driving these cloud particles upward, sort of like a volcano bringing up material from the depths and making it visible from outside the atmosphere,” explains Sromovsky, a senior scientist at UW-Madison and an expert on planetary atmospheres. “The upper haze is so optically pretty thick that it is only in the stormy regions where the haze is penetrated by powerful updrafts that you can see evidence for the ammonia ice and the water ice. Those storm particles have an infrared color signature that is very different from the haze particles in the surrounding atmosphere.”

Scientists believe Saturn’s atmosphere is a layered sandwich of sorts, with a deck of water clouds at the bottom, ammonia hydrosulfide clouds in the middle, and ammonia clouds near the top, just below an upper tropospheric haze of unknown composition that obscures almost everything.

The latest great storm on Saturn and the presence of the Cassini probe now orbiting the planet gave scientists a chance to peek beneath the haze and learn more about the dynamics and chemical composition of the planet’s deep atmosphere.

First noticed by amateur astronomers, the massive storm works like the much smaller convective events on Earth, where air and water vapor are pushed high into the atmosphere, resulting in the towering, billowing clouds of a thunderstorm. On Saturn, not only are the storms much bigger, they are far more violent, with models predicting vertical winds of more than 300 miles per hour for these rare giant storms.

The effect, Sromovsky says, is to loft the aerosols found deep in the atmosphere to the visible cloud tops, providing a rare glimpse of normally hidden materials. “It starts at the water cloud level and develops a huge convective tower. It is similar to a big thunderstorm, only 10 to 20 times taller and covering an even greater area,” he explains.

The new work helps validate the models of Saturn’s great storms as well as previous observations that detected water and ammonia in vapor form. The presence of water ice, he says, supports the idea that Saturn’s superstorms are powered by condensation of water and originate deep in the atmosphere, about 200 kilometers below the visible cloud deck.

“The water could only have risen from below, driven upward by powerful convection originating deep in the atmosphere. The water vapor condenses and freezes as it rises. It then likely becomes coated with more volatile materials like ammonium hydrosulfide and ammonia as the temperature decreases with their ascent,” Sromovsky adds.

The interesting effect, he notes, is that in Saturn’s massive storm, at least, the observations can be matched by having particles of mixed composition, or clouds of water ice existing side-by-side with clouds of ammonia ice. In the latter scenario, water ice would make up 22 percent of the cloud head and ammonia ice 55 percent. The remaining fraction would be made up by the third constituent, which though less certain, is believed to be ammonia hydrosulfide.

“Up until now, there have been no quantitative calculations of spectra for cloud structures and compositions that matched the observed spectrum of an actual storm cloud feature,” says Sromovsky.

Via University of Wisconsin



The Yukon’s Northern Lights from Phil Hart

Categories: Education

The Yukon’s Northern Lights from Phil Hart on Vimeo.

My three favourite things in the world are mountains, aurora and snow. In early 2012 I got all three of them in spades when I spent nine weeks in the frozen north of Canada’s Yukon Territory, thanks to the generosity of my hosts Andrea and Florian Lemphers.

With four cameras and dozens of lenses, tripods and a truck full of extreme cold weather gear, I journeyed across the Yukon and chased every gap in the clouds I could find. Three terabytes and a long learning curve later, this video is short compilation of some of the best footage I captured during my aurora adventures.

Details about this video:

Cameras: 2 * Canon 5D Mark II, Canon 1100D (aka Rebel T3), Canon 5D.
Lenses: Canon 24mm f1.4L I & II, 14mm f2.8L, 10-22mm f3.5-5.6.

Motion Control: Vixen Polarie, Dynamic Perception Stage Zero Dolly and a custom controller developed jointly with Fred Vanderhaven which provides pan/tilt motion control and most importantly almost fully automated day-to-night twilight exposure control. The automated aspect is particularly important in the Yukon – a long twilight at -30 degrees means you can’t be standing by adjusting the camera the whole time, especially when there are three other cameras to operate.

Processing: RAW image sequences have been processed using Lightroom and LR Timelapse, then rendered with After Effects and Premier Pro.

You can read more about my adventures in the Yukon on my blog:

I set my talented friend Dean Roberts (of ‘The Dirt Floor’ band and ‘Lithostylis’ wines) the challenge of recording music for the video. I hope you enjoy the rockin’ soundtrack he came up with.

Phil Hart
31st May 2013


Annular Eclipse 10th May 2013

Categories: Education, Members

On the morning of Friday 10 May  an annual or partial eclipse will pass across northern Australia.

In Sydney, the eclipse begins at 7.50 am reachng 39% coverage of the suns face at 8.57am and ending at 10.14am. The Sun will be 24 degrees above the eastern horizon which should provide reasonable viewing for most observers. The further towards teh tropic of Capricorn you are, the greater the eclipse will cover the sun. Being an annular eclipse, the sun will not be totally blacked out and is therefore dangerous to observe without filtered protection throughout the entire event.

The eclipse can be safely viewed using a telescope equipped with a specialised solar filter or simply projecting the image through a small telescope.  Cardboard framed ‘eclipse glasses’ meeting international standards are also safe to use if their instructions are followed.  Suitable ‘eclipse glasses’ are available locally from reputable astronomy shops, public Observatories and Planetaria.

More information about the eclipse and safe ways to view it can be found in a Factsheet produced by the Astronomical Society of Australia (ASA).  The sheet has been posted on the ASA’s Australian Astronomy web site (  The  Factsheet  link is:  You may wish to use this sheet to inform friends, students or the public about this event.  The sheet may be freely copied for wide distribution provided the Australian Astronomy and ASA logos are retained.



Quasars with Prof Ron Ekers

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Last month, Professor Ron Ekers present a free lecture at Curtin University to commemorate the publishing of the discovery of Quasars.


I’m please to let you know we’ve got the final edit of the “Quasars – from the Milky Way to the Edge of the Universe with Prof Ron Ekers” up on youtube and ready to be share with anyone who would be interested. 


“On March 16th, 50 years ago, a joint effort between Australia and the USA led to the discovery of Quasars and fundamentally shifted our thinking about the Universe. This is a fascinating story of scientific debate, monumental leaps in knowledge, and global cooperation.

Professor Ron Ekers speaks about what we’ve learned over the past 50 years of peering into space and where we might go next with telescopes such as the Square Kilometre Array.

Professor Ekers has worked with some of the world’s most renowned astronomers at some of the top University’s and Observatories including Cal Tech and the National Radio Astronomy Observatory in New Mexico.

He was elected a Fellow of the Australian Academy of Science, a Foreign Member of the Royal Dutch Academy of Science, a Foreign Member of the American Philosophical Society and a Fellow of the Royal Society. He’s a past President of the International Astronomical Union (IAU) and a member of the Advisory Board for the Peter Gruber Foundation Cosmology Prize.”



Introduction to Astronomy Course

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If you are interested in Astronomy and have often wondered how you could learn more, the Duke University is offering a free course via an on-line medium called Coursera.

This innovative educational network of Universities providing free courses from a broad range of subjects and topics. The Coursera web site describes themselves as “…a social entrepreneurship company that partners with the top universities in the world to offer courses online for anyone to take, for free. We envision a future where the top universities are educating not only thousands of students, but millions. Our technology enables the best professors to teach tens or hundreds of thousands of students.Through this, we hope to give everyone access to the world-class education that has so far been available only to a select few. We want to empower people with education that will improve their lives, the lives of their families, and the communities they live in.”

The course that is of the greatest interest to us is the “Introduction to Astronomy” course provided by Duke University, North Carolina. In this class, “we will be studying, quite literally, everything in the universe.  We will start with “classical” astronomy, describing the night sky and organizing what we see as was done in ancient times.  We will then embark on a journey, starting here on Earth and progressing outward, to study the Solar system, the Milky Way galaxy, and the wonderful and strange objects we observe in deep space, such as black holes, quasars, and supernovae.  We will end with some discussion of what scientists know today about the universe as a whole.  Along the way we will introduce some of the methods, theoretical and experimental, that have been used to understand all of this, from Newton’s laws, through our understanding of light and matter, to Einstein’s theory of relativity, and from Galileo’s telescope to WMAP.”

This nine week course is 100% on-line making it accessible to virtually everyone who has access to the internet. Requiring a medium level of mathematical and physics knowledge is the only prerequisite, with a certificate of completion offered at the successful completion of the course. The availability of free education is quickly becoming a thing of the past. With Coursera offering this opportunity for free education world wide there is an incentive for many students and would be students to continue further education throughout their life.


Before & After the Solar Eclipse Cairns 2012

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By Dan Crowley

After arriving at Cairns on the Monday night, we rose early on Tuesday morning to view the eastern horizon from our hotel room. We had specially booked this room with the intention of setting up our cameras on the balcony and waiting in comfort for the eclipse to unfold. Before sunrise, the dark sky reveal only a few stars directly overhead. To the east a mountain stood between us and the sun. Although not an ideal location, the determined altitude of the sun at totality being 14 degrees would theoretically place the sun  above the crest of the small volcanic landscape. The unpredictable and threatening aspect of the setting was the cloud cover that hung perpetually over the hills. As the sun began to rise we were not able to find its position due to being completely blanketed by black stormy clouds. A small gap appeared intermittently allowing sun beams to radiate onto the buildings along the wharf.

As part of our contingency plan, we had a day before the eclipse to research the weather conditions and possible alternative locations. Some associates and friends that we had dined with the previous night elected to seek out a location near their accommodation. They decided on Trinity Beach being twenty kilometres north of Cairns CBD it provided good veiw of the ocean and was not far from their caravan park. The only problem was it was one of the popular locations for film crews and organised groups to assemble. These suburban locales were closed off to traffic an hour before totality so as to limit the traffic into the area. We thought more options would make themselves known once we drove further north. Having the whole day ahead of us, we journeyed north along the Captain Cook Highway, passing Palm Cove and Port Douglas along a stretch of road that closely passes the ocean beaches with their mixture of sedimentary sandstone and igneous granite rock facings. We found a number of good possibilities with good parking close to the beach and clear easterly views of the ocean. Stopping at a few of these locations, we checked our bearings with our smart phone compass and declared this area to be our best option for the eclipse morning. The rest of the day was filled with visits to the Daintree Discovery Centre and a drive to the furthest northern point on the sealed road at Cape Tribulation. On our return trip we scouted for any better locations considering Port Douglas as an alternative choice as the centre line of the shadow was some where south of this bustling tourist town. Not wanting to be forced to find parking at shared beaches, we revisited the place we had selected on the way up. Ellis Beach is 7 kilomtres north of Trinity Beach and Yorkey’s Knob and a few kilometres north of Palm Cove. This long expanse of coastal beach provided numerous vantage points with plenty of space for the potential hundreds of visitors that were do the same as we were. Many people were already setting up camps along the road, claiming their position as the afternoon went on. After returning to our hotel and balcony, the cloud was still hanging over the east so our minds were set to leave early the next morning and head north.

At 4 am on Wednesday 14th November 2012, we prepared for our journey; having breakfast, gathering tripods and cameras, then packing our hire car we left for the north coast. Arriving at Ellis Beach around 5 am, there were a large crowd already gathered on the beach. We picked  our spot before the sun was above the horizon and set up the cameras. To our dismay there was a thick band of cloud settled above the ocean. Next to us were a couple of Frenchmen along side a family of Ukrainians now living in Melbourne. Brent, a local plaster sat beside us with his cross German Shepard and Stafford-shire  Terrier wondering what the fuss was all about.

The sky began to lighten revealing a bank of low cloud along the ocean horizon. We estimated the point where the sun would rise a little east off the point as the beach faced a more northerly direction. The glow in the horizon surprised us a little to find the rising sun closer to the point than we expected. Nevertheless we still had a perfect view of the sunrise as it broached the horizon like a golden fire spreading across the eastern sky. A scattering of cloud provided a beautiful contrast with the only exception that these cloud were moving into crowd out our sun. At this point we had some concern that the cloud cover was increasing in magnitude inhibiting any vision of the first contact of the sun and moon at 5:44 am. We would miss the beginning of the eclipse process where the moon slowly passes in front of the sun blocking its face and creating a diminishing crescent shape in its passing. This was not such an  important issue as there was forty minutes left until second contact begins. A few mobile phone calls to our colleges at Trinity Beach confirmed that they were experiencing the same cloud cover. With twenty minutes to go the sky was patchy with cloud and there was a chance that the sun would not reveal itself in time. To the north towards Port Douglas, the sky appeared to be clearer but the percentage of cloud was 50% as was the sky east of our beach. There was no point changing locations at this late stage and we sat tight waiting with baited breath as the clock countered down towards the predetermined moment.

Within a minute of the totality, the clouds opened up to reveal the final stage of the first event. A crescent shaped sun appeared through a window in the cloud. the excitement along the beach could be heard as a synchronized sigh of relief was released and anxiety levels percolated  into a feeling of joyful resound. The encroaching shadow was darkening the early morning sun creating an iridescent purple glow to the sky. The temperature dropped a few degrees and the atmosphere retained an eeriness reminiscent of medieval tales of witchcraft and sorcery.  The cloud parted ways within a minute of the moon’s enclosure of the suns surface as the sky darken into twilight making it difficult to read the settings on my camera. Alas I had forgotten to bring a red light torch so I was forced to make guess work of my desired settings. At this point I was taking photographs with my Canon D40 camera via a 2x extender and a Canon 100 to 400mm EF zoom 77mm lens giving me a 800mm telephoto view of the sun through a white light filter. Quickly removing the filter seconds before the second contact began there was time to capture the final 30 seconds of teh sun before totality. The cameras aperture struggled to process the shots with the quickly changing light levels.

A voice behind us countered down the moment, 5..4..3..2..1..A cheers went out along the entire beach. The moon engaged the sun by completely covering its face to reveal a blazing corona. The halo of light sparkled and danced around the edge of the moon as people stood in awe of this pnenominia ong the coast.

Cameras clicked and flashes erupted as hundreds of cameras attempted to capture the experience. Birds that normally would have been actively foraging, nestled themselves chirping and calling their mates to roost. For two minutes the shadow remained on the beach holding the focus of its occupants skyward. My view of the eclipse through the eyepiece of my camera enhanced the solar flares and prominences with their rich red coloured projections extending thousands of kilometres beyond the surface of the chromosphere. Not needing any filtered protection to view this event, observers studied the suns corona and its extended solar winds with the naked eye now visible around the edge of the moon.

Two minutes passed quickly as the moon moved away and the sun returned to shine beyond the edge of the luna satellite. The curve of the moon allows a flash of sun beams to sparkle beyond is surface, bending around the edge of its crators creating an effect known as the Diamond Ring. The glowing pinch of light begins to spread across the lunar circumference quickly growing in intensity until it becomes too bright to view with the naked eye. The third stage of the eclipse begins as the moon moves away and the crescent shape of the sun reappears and increases over the next 40 minutes. Brent, our local plasterer is beside himself having experienced what he discrbes as a biblical event that for many will be the first and only time they will see it in their life. He was so pleased he had decided to come out to witness this before work,  stopping on what would normally be a quiet and secluded beach scape on the side of the highway.

Making a phone call to our friends at Trinity Beach to share the experience, we discovered that they had not seen any of the totality due to the persistent cloud cover. It was almost impossible to imagine that seven kilometres south, the cloud could be so different to where we had been positioned. Within a few minutes a car pulled up and an American tourist from Arizona stepped out to see how our viewing had worked out. He explained that he had passed out position twenty minutes earlier and decided to travel a few kilometres north where he thought the cloud was thinner. They had missed the beginning of the first stage as we had but also missed part of the second stage as the cloud cleared for them just after the totality began. As the crowd dispersed we logged our observations on Facebook and emailed members at home before  we packed our cameras and tripods away. We drove north to Port Douglas in search of a shop for morning tea and spoke to a couple from the Netherlands who had rendezvoused on the northern end of Port Douglas Beach. Apparently the cloud cover there was almost as bad as Trinity Beach only seeing the last half of totality. Another passer by said he was at the southern end of the beach and had 100% advisability of the event. No matter how much research and good preparation you may do before hand, there is always a risk of failure when choosing a place to observe an eclipse. Of all the places we had available to chose, we were just lucky to pick a spot that provided the clear skies at the right time.

This event only occurs because the size of the moon is exactly the same apparent size of the sun. Such a coincidental ratio of star and satellite possibly never occurs anywhere else in the universe. We consider ourselves fortnate and lucky to be have witnessed this event for the third time and hope it won’t be out last.


2012 Solar Eclipse Cairns

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Solar Eclipse: Northern Queensland

14th November 2012


On 14th November 2012, Australia will again experience the shadow of the moon as it passes between the Sun and the Earth. This event (second contact) will occur at 20:38UT on November 13th which translates to 6:38 am Australian Eastern Standard Time on 14th November due to the difference in the time zones.

The first point of contact for the shadow will be in the Northern Territory on the north east boarder of Kakadu National Park near Ubirr Rock. The path of the shadow will continue east across Arnhem Land, crossing the Gulf of Carpentaria then onto the Cape York peninsula near Wallaby Island. From here the shadow will progress south east crossing the eastern coast of Queensland 30 km north of Cairns.

Cairns and Port Douglas will provide some of the best viewing areas as they are populated tourist destinations providing ample accommodation and services. At the time of totality, the sun will have risen 14° above the horizon when it will last for two minutes.

As sunrise on the day will be approximately 5:35am, there is an hour available to find the best location for your observation point. there is the option to drive up or down the coast to find the best location north of Port Douglas, where their are open fields and places to stop with many other eclipse chasers. This require a bit of planning the day before as an early start in the dark will make it difficult to see what the cloud cover looks like. My suggestion is to find a comfortable spot on the balcony of your Resort room with a hot breakfast delivered to your room. All-in-all, coast observers might be better advised to sit and take whatever nature offers, as no matter what decision you make it will be just as good as any other on the day.

A total solar eclipse forms a rare opportunity to observe the corona (the outer layer of the Sun’s atmosphere). Normally this is not visible because the photosphere is much brighter than the corona. According to the point reached in the solar cycle, the corona may appear small and symmetric, or large and fuzzy. It is very hard to predict this prior to totality.



Phenomena associated with eclipses include shadow bands (also known as flying shadows), which are similar to shadows on the bottom of a swimming pool. They only occur just prior to and after totality, when a narrow solar crescent acts as an anisotropic light source

When the shrinking visible part of the photosphere becomes very small, Baily’s beads will occur. These are caused by the sunlight still being able to reach Earth through lunar valleys. Totality then begins with the diamond ring effect, the last bright flash of sunlight.

It is safe to observe the total phase of a solar eclipse directly only when the Sun’s photosphere is completely covered by the Moon, and not before or after totality. During this period the Sun is too dim to be seen through filters. The Sun’s faint corona will be visible, and the chromosphere, solar prominences, and possibly even a solar flare may be seen. At the end of totality, the same effects will occur in reverse order, and on the opposite side of the Moon.

Under normal conditions, the Sun is so bright that it is difficult to stare at it directly. However, during an eclipse, with so much of the Sun covered, it is easier and more tempting to stare at it. In fact however, looking at the Sun during an eclipse is as dangerous as looking at it outside an eclipse, except during the brief period of totality, when the Sun’s disk is completely covered (totality occurs only during a total eclipse and only very briefly; it does not occur during a partial or annular eclipse). Viewing the Sun’s disk through any kind of optical aid (binoculars, a telescope, or even an optical camera viewfinder) is extremely hazardous and can cause irreversible eye damage within a fraction of a second.

Looking directly at the photosphere of the Sun (the bright disk of the Sun itself), even for just a few seconds, can cause permanent damage to the retina of the eye, because of the intense visible and invisible radiation that the photosphere emits. This damage can result in impairment of vision, up to and including blindness. The retina has no sensitivity to pain, and the effects of retinal damage may not appear for hours, so there is no warning that injury is occurring.

Photographing an eclipse is possible with fairly common camera equipment. In order for the disk of the Sun/Moon to be easily visible, a fairly high magnification long focus lens is needed (at least 200 mm for a 35 mm camera), and for the disk to fill most of the frame, a longer lens is needed (over 500 mm). As with viewing the Sun directly, looking at it through the viewfinder of a camera can produce damage to the retina, so care is recommended.

For more detailed information on eclipse photography visit:





Transit of Venus 6th June 2012 by Gerard Keyzer

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This is a gentle reminder of a truly rare event that is on our horizon. This month’s Astro Flier will be our last
publication prior to this celestial wonder so you need to be prepared. For night- time observers, on other pages in the magazine I have reprinted – with kind permission of Geoff Smith, Observations Officer of the ASNSW, an observing list he published for the South Pacific Star Party. The list is entirely relevant to our sky for the next month or so, bearing in mind that the time advances by two hours per month (completing a full circuit in a year) and the area of sky will move 15 degrees further west than at the same time last month.

Jupiter is moving completely behind the Sun from the Earth and as such is no longer a viable target. Mars of course is easy to find near Regulus in Leo and for all its’ tiny apparent diameter is shining like a bright ruby at mag. 0.2. Saturn has also passed opposition and is in our northern sky throughout the night. It is imperative that we take advantage of the steady seeing and dustless skies to view the celestial beauty of this gas giant, we had to wait six months as we will now have to await the return of Jupiter. Venus is moving in front of the Sun next month!

The Transit of Venus on 6th June is perfectly timed for Eastern Australia and we get to see the whole event as it lasts 6½ hours. This means that even should cloud obscure our view the chances are we will see at least some part of the event. We have had a brief outline of the historical significance at an earlier meeting but it is personally significant to all of us as we will never see it again (I would have to live until I was 159 years old! Jack will be 187!) Anyone who doesn’t catch a glimpse this time will not see it ever, nor will 95% of people born this year.

Scientifically speaking this Transit commemorates one of the first real global and multilateral
scientific endeavours, one that was not primarily based on the desire for profit, but more the
advance of knowledge.

In 1619 Johannes Kepler, mathematician and astronomer, had used the meticulous observing
notes of Tycho Brahe to formulate his Three Laws of Planetary Motion. The Third law, which
concerns us here, tells us that the cube of a planet’s mean distance from the Sun is directly proportional
to the square of that planet’s orbital period. The orbital periods of the planets were easily calculated,
even by naked eye observers lacking truly accurate measuring tools. By using the Third
Law and the length of the Venus year they knew that Venus’ distance from the Sun was 72.3% of
the Earths’ distance.

If astronomers had a way of measuring one such distance accurately, the distances to all the planets could readily be calculated. Once the distances were known, the planets apparent size (angular) could be measured and the actual size could be calculated. Once the actual size of a planet was known, the orbits of that planets’ moons could give us the true mass of the planet. Astronomers were taking tentative steps on the second stage of measuring the local universe. But most importantly, if the true Earth – Sun distance could be calculated, we could begin to measure, using parallax, the distance to the nearest stars!

Parallax is the apparent shift in an objects position when viewed from different angles. In its’ simplest form our paired eyes use parallax to gauge the distance of objects we view. In astronomical terms it was seen as a means to measure the distance to the nearest stars. If an object was observed at six month intervals to move against the background of distant stars the angle could be calculated and the distance extrapolated. The baseline of the triangle would be the diameter of the orbit of Earth or twice the Earth-Sun distance.

Sir Edmund Halley, in 1677, proposed that it would be possible to calculate the Venus-Sun distance
by using the same principal if the Transit was viewed from two widely separated locations on Earth. Well
planned, well funded, well staffed, and well provisioned expeditions set off at the behest of the major European
powers to observe the Transits of 1761 and 1769. The British expedition to Tahiti, led by Lieutenant
James Cook, led to the mapping of New Zealand and the east coast of Australia. The expeditions met with
varying degrees of success, encountering issues such as cloud, local hostility, harsh conditions of travel, poor
navigation (positioning of observer) and timing issues. As well as inaccurate timepieces that were used to
calculate longitude, they also experienced “ the Black Drop”, blurring of edges due to the atmosphere and
poor optics, that affected the precise recording of the ingress and egress time that was essential to the parallax measure. Nevertheless, when all the data was collated and calculations were made, the results gave a figure within 3% of the distance known today!

The Transit we will Observe

The Transit begins when Venus appears to move on to the surface of the Sun and this is due at 8:16 am in
Wollongong, one second later than in Sydney. The most significant timing is ingress, interior or second contact, occurring at 8:34 am. I suggest being well set-up by 7:30 am with a clear view of the east. A comprehensive article appears on pp 8,9, 10 of Astronomy 2012 For most of us the safest way to view is by projecting the solar image . This view can be shared with many bystanders and the image can be easily
photographed by individuals. A music stand to hold your target screen would be useful.

SAFETY! Do not look at the Sun through any optical device without full aperture solar filter at the
objective end of the scope!
These are available from any astronomical supply shop and fit completely over the dew shield. SECURE IT
IN PLACE. If you project the Sun image remember that unprotected sunlight will heat the inside of any scope tube in minutes, will melt any adhesives between lenses, ruin eyepieces and burn anything in its way. If your eye gets burned, you will be blinded.

For those of you imaging, make sure the project is well planned. While the Transit lasts a long time, critical stages don’t last more than a few seconds. I suggest trying to photograph first and second contact, and/or third and fourth contact with a few shots in between. More experienced astrophotographers could take a shot every 10 or 15 minutes and create a sequence later on. One of the best things you can do is photograph
the occasion, i.e. the equipment, other viewers and friends, and the location. These will be your lasting memories. There will be thousands of photographs taken that will be better than yours so ABOVE ALL, DON’T WORRY, enjoy the occasion and the spectacle. You will be playing a small part in the history of astronomical observing.
I will be observing first and second contact from my observatory in Kangaroo Valley and then going to the KV Showground at 10 am to show interested locals. After that it’s off to a local High School so feel free to contact me if you want to join in.

Clear Skies


April 2012 Observation Report by Gerard Keyzer

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Star Stuck

Has the rain stopped? It didn’t even rain at Easter (except in Sydney somewhere, and Melbourne of course). Cool dry evenings and the end of daylight savings mean you can get out observing quite early. The lack of dust and moisture in the air make observing conditions excellent, while the lack of heat means turbulence is minimal. If you can brave the cold, the next six months are the best time of year for amateur observers.

So, what’s happening? Firstly don’t forget there is a Transit of Venus on June 6th. If anyone wants to get some advice about observing the Sun safely please contact me on       More immediately the best planet for us to view is beautiful Saturn.  Saturn transits the meridian on April 16th (due north at local midnight) and is rising around sunset. As such, Saturn is perfectly placed for viewing throughout the night. With a modest telescope and medium magnification you should be able to see the shadow of the rings on the planet and perhaps even the dark ring dividing the two bright rings known eloquently as the A ring and B ring. Who says astronomers have no imagination? This is known as the Cassini division after its discovery in 1675 by Giovanni Domenico Cassini. The rings can even be seen in 10x binoculars if they are mounted on a tripod or held steadily. Saturn has five moons that may be seen in progressively larger telescopes but even binoculars will allow us to find Titan, which is actually the largest of all moons in the solar system, having a diameter of 5,152 klms. Saturn resides in the constellation Virgo for all of 2012 and is currently just north of the 1st magnitude star Spica, αVirginis. Spica will appear quite white and Saturn very yellow. There are few other bright stars in this area but Mars is just over the border in Leo near the bright star Regulus. Mars will appear a rusty orange colour and Regulus more yellow-white. Regulus marks the resting foreleg of Leo, the mythical Lion. Mars is actually shining brighter than Saturn but is quite small. I would be interested to hear of anyone perceiving any detail on this enigmatic planet.


For the deep sky observers, Virgo and the adjacent constellation Leo are veritable goldmines of galaxy fields. As a matter of fact a supernova was discovered on March 16th in the galaxy M95 in Leo.  Currently this end of life stellar explosion is shining with the light of 500 million Suns! It is still invisible to the naked eye and actually happened 38 million years ago, its light only reaching us just now. M95 is part of a well known trio of galaxies with, M96 and M105, all visible in one low power field. Its coordinates are RA 10 44m Dec =11° 42’

M95 and the Supernova designated SN 2012aw : Image Credit: Anthony Ayiomamitis

Above we see an image of the entire galaxy field in Leo taken by my friend Bob Price from Bethanga, in Victoria. Six galaxies appear in total with one unnamed. M95 is in the bottom right of the image with the SN showing just below to the right and some glare from nearby Mars bleeding into the pixels from the right.

 This SN and galaxy is easily visible in a 150mm telescope and Leo is currently in our north, about 35° up the sky.

 Although they are the natural result of the end of life cycle of a massive star, supernovae are relatively rare. Only three are known to have occurred in our Milky Way in the last 1000 or so years. The first occurred in Taurus and was recorded by Chinese and Middle Eastern astronomers around 1054 A.D. It’s remnant is the famous Crab Nebula, M1. The next was discovered and observed in 1572 by the Danish Astronomer Tycho Brahe, in the constellation Cassiopeia, it became known as Tycho’s Star.

Below: Tycho’s Star as recorded in his observing notes. It is designated I and called Nuoa Stella, New Star. As you can see it appeared very bright

The most recent was SN 1987a in the Large Magellanic Cloud (strictly speaking not in our galaxy but in our galactic neighbourhood). It was actually discovered by radio astronomers, three hours ahead of being discovered visually, simultaneously in Chile and New Zealand.

 It is now a brilliant planetary nebula with the typical hourglass shape created by the expanding rings of gas shown end on.


Clear Skies

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