Archive for the ‘Other stuff’ Category

How to calculate your horizon distance

May 25, 2015 2 comments

While on a recent trip to the remote South Atlantic island of St Helena (exile place of Napoleon, and location of Edmond Halley’s observatory) [blog post to follow!] I ascended the highest mountain on the island, Diana’s Peak.

At 823m above sea level it commanded splendid views of the island, but the most striking thing was the unbroken 360° view of the horizon. I did a quick calculation in my head of how far I could see, and that forms the basis of this blog post: how do you calculate your horizon distance?
It turns out it’s pretty straight forward if you know a little simple maths. It helps to start by drawing a picture, so I did:
Definitely not to scale

Definitely not to scale

For an observer of height h above sea level, the horizon distance is D. The Rs in this diagram are the radius of the planet you’re standing on, in this case the Earth. The only real assumption here is that you’re seeing a sea level horizon.As you can see you can draw a right-angled triangle where one side is D, the other is R, and the hypotenuse (the side opposite the right angle) is R + h.

Using Pythagoras’s Theorem, discovered around 2500 years ago, the square of the hypotenuse is equal to the sum of the squares of the other two sides. So we can say that:

(R + h)2 = R2 + D2

If you expand the part to the left of the bracket you get (R + h)2 = R2 + 2Rh + h2 so that:

R2 + 2Rh + h= R2 + D2

There’s an R2 term on both sides of the calculation so you can cancel them out, leaving:

2Rh + h= D2

Therefore the horizon distance, D, is:

D = √(2Rh+h2)

Here’s where you can make life much simpler for yourself. In almost every case R is much, much larger than h, which means that 2Rh is much, much larger than h2 so you can just ignore h2 and your equation simplifies to:

D ≈ √2Rh

(the ≈ sign here means “almost equals”. Honestly.)

So if you know R and h you can calculate D. To make this calculation easily you can carry round the value of √2R in your head meaning you only have to calculate √h and multiply those two numbers together.

So for the Earth, R is 6371000m, so √2R is 3569.6. Multiplying this by √h in metres would give you D in metres, so lets convert that into km to make things easier. This means dividing this number by 1000, giving an answer of 3.5696 which is ≈ 3.5.

So as a rough rule of thumb, your horizon distance on Earth,

D = 3.5 x √h

where D is measured in km and h in metres.

On Diana’s Peak, at 823m high, √h = 28.687… which multiplied by 3.5 gives a horizon distance of almost exactly 100km!

This is pretty cool, and is true of anywhere you can see the sea from a heigh of 823m.

One final calculation which sprung to mind on the mountain top was the area of sea I could see, which is easy to work out using the fact that the area of a circle is πr2, where r in this case is D, or 100km.

π is 3.14159 which means that the area of sea I could see was 31415.9 km2. Just a tad larger than Belgium, at 30528 km2.

And in that Belgium-sized circle of ocean was only one ship, the RMS St Helena that was taking me home the following day.

What about on other planets?

If you’re on Mars your horizon distance is shorter, at 2.6√h. On Mercury it’s smaller still at 2.2√h. This is due to Mars and Mercury being much smaller than the Earth, and so their surfaces curve away from you quicker. Venus is almost exactly the same size as the Earth (only a fraction smaller) so there you’d have to use the same calculation as here on Earth, 3.5√h.

Hovering above the surface of Jupiter your horizon would stretch to 11.8√h and on Saturn to 10.8√h. Uranus and Neptune are about the same size, giving a horizon distance of 7.1√h.

Mercury 2.2√h
Venus 3.5√h
Earth 3.5√h
Mars 2.6√h
Jupiter 11.8√h
Saturn 10.8√h
Uranus 7.1√h
Neptune 7.1√h

What about the dwarf planets? Being so small their surfaces will curve away from you very quickly, shortening your horizon distance. One of the smallest spherical objects in the solar system is the dwarf planet Ceres (as in cereal), which is the largest object amongst the fragments of rock in the asteroid belt. Your horizon distance on Ceres is almost exactly √h, making that a pretty simple horizon calculation!

John Dobson, “The Sidewalk Astronomer”, 1915-2014

January 16, 2014 2 comments

John Dobson, known as “the sidewalk astronomer“, and the inventor of the Dobsonian telescope mount, died yesterday 15 January 2014.

John Dobson, 1915-2014

John Dobson, 1915-2014

I had the pleasure of meeting John back in 2006 when he visited Glasgow Science Centre to give a talk in the planetarium. As planetarium manager at the time I was in John’s company for most of the two days he was in Glasgow, and became well used to his unorthodox – and mischievous – teaching style.

“How many stars are there in our solar system?” he asked, with a twinkle in his eye.
“One…?” I ventured, smelling a trap.
“Actually there are three. Jupiter and Saturn are stars too. They define a star as something that emits visible light. But Jupiter shines in infra-red; it gives off more than twice what it takes from the sun, but astronomers don’t see that, because they’re too retarded. You see, that’s the problem with talking to me – I throw you a curve ball.”

His most controversial views were regarding the Big Bang Model. It’s fair to say that John wasn’t a believer* – he told me he was “allergic” to it! He instead promoted a steady state model, where the receding galaxies “fell off the edge” and got recycled back in… To be honest I didn’t really follow his arguments too closely, but there’s no doubting the entertainment of his delivery.

Certainly the audience who came to Glasgow Science Centre’s planetarium to see John talk were thoroughly entertained. Perhaps not in a very orthodox way, nor with theories that were widely accepted in the astronomy community, nor indeed about what they thought they’d hear John speak about. The talk had been billed as “hear John Dobson, inventor of the Dobsonian telescope mount, talk about his revolutionary design and his passion for sidewalk astronomy”. He gave that five minutes at the start of the talk; the rest was non-standard cosmology and poking fun at the consensus.

He didn’t credit himself as the inventor of the Dobsonian mount. After all, astronomers had been using elements of it for a long time before John put them all together and began popularising this low-cost mount.

A Dobsonian Telescope Mount

A Dobsonian Telescope Mount

A Dobsonian mount is effectively a spinning plate with a cradle on it for holding the telescope. The plate spins allowing you to move the telescope from side to side (the azimuth co-ordinate, in astronomy speak) and the telescope can tilt in the cradle allowing you to move it up and down (the altitude co-ordinate). This is a far simpler mount than the alternatives, and can be built out of everyday items at low cost, meaning that more of your budget can go on the telescope tube itself, building larger tubes to collect more light (we call these large telescopes “light buckets”) and so get clearer, sharper images.

John himself never called them Dobsonians, instead referring to them as “sidewalk telescopes”. “For hundreds of years, wars were fought using cannon on ‘Dobsonian’ mounts; it’s nothing new,” he would say. But his design was innovative, and it brought the universe a little bit closer to us.

My primary telescope – the Skywatcher 250 PX – uses a Dobsonian mount. It’s an ideal scope for public astronomy events as it’s very quick to set up, and is really easy to operate. Want to move it? Just nudge or pull it.

John’s mount, and his passion for showing people the universe through a telescope, led to his popularising of “sidewalk astronomy”, which involves standing with a telescope out in a busy street in your town and showing passers-by views of the cosmos. Of course due to light pollution in towns and cities you’re limited as to what you can show, but the Moon and planets are easily visible from wherever you are. If your unsuspecting passer-by has never seen the rings of Saturn, or the moons on Jupiter, or mountain ranges and craters on our own Moon, you can be sure that their few minutes with your telescope will amaze them.

John Dobson will be remembered as the grandfather of sidewalk astronomy, but I’ll remember him most fondly as the very eccentric and enthusiastic man that I spent a couple of days with in Glasgow in 2006. The most vivid memory I have of John is taking him out for dinner the night he arrived in Glasgow, as I did with all visiting speakers. He didn’t eat meat, he informed me. And he didn’t eat processed food in restaurants. He saw that I was beginning to look worried. I suggested he might like a salad. With a grin he said “Why pay for a salad when there’s perfectly edible stuff just laying around?”, at which point he began rummaging in the flowerbeds for edible plants and weeds…
* Not that I’m a believer. I don’t believe in the Big Bang, rather I accept it as a model for the universe which fits all of the observations that we make. It’s true, to the limits of our current observations.

Light Pollution and Birds: Early Bird Survey

January 8, 2014 Leave a comment

The negative effect of light pollution on wildlife has long been known, specifically – but not exclusively – its effect on bats, bugs, and sea turtles. Now the British Trust for Ornithology (BTO) are running an Early Bird Survey, asking people in the UK to monitor the pre-dawn feeding times of garden birds to see what – if any – effect light pollution is having.

To take part you need to get up before dawn* on 9** January 2014 (tomorrow, as I write this), watch your garden bird feeders, and record the times that the first ten species arrive to feed. You can download the full instructions here (pdf), and submit your observations here.

* dawn occurs at different times around the UK, so you should find your sunrise time and get up half an hour earlier than that, during civil twilight.
** observations on 10, 11, and 12 January are welcome too.

As the BTO website says:

Winter is not an easy time for birds. They need extra energy to keep warm, especially during long winter nights. To cope with this, they lay down extra fat reserves, though small birds quite often only lay down enough for a single night. Longer nights not only affect the amount of energy a bird uses, they also reduce the amount of time that birds can feed in. Birds, therefore, have to make the most of the daylight hours to replenish their energy reserves before it gets dark.

The 2004 BTO Shortest Day Survey, run in association with BBC Radio 4, investigated the patterns behind birds arriving at garden bird feeders first thing on a winter’s morning. Building on observations from the Shortest Day Survey, the Early Bird Survey will investigate what effect, if any, light and heat pollution have on the feeding patterns of birds during a cold winter’s morning.

Scots in Space

I was delighted to hear that two groups from Glasgow were winners in last night’s UK Space Conference‘s Arthur Clarke Awards 2011.
Clyde Space, a “leading supplier of small and micro spacecraft systems”, was given the Arthur Clarke Award 2011 for Achievement in Space Commerce, while the University of Strathclyde’s Advanced Space Concepts Laboratory, which “undertakes frontier research on visionary space systems”, was given the Arthur Clarke Award 2011 for Achievement in Space Research.

Congratulations to both, and it’s exciting to me as a Scot and a resident of Glasgow that these two groups, located within 5 miles of one another, are leading the UK in space research and commerce.

The Circle of Little Animals

December 3, 2010 Leave a comment

This is an auspicious time of the year.

The Sun, on its yearly circuit of the sky*, moves gradually along the ecliptic, a line which is the projection of our solar system’s disk onto our night sky. This line, the ecliptic, is also known as the zodiac, a term originating from the late 14th Century, and deriving from the Greek literally translating as “circle of little animals”. (Incidentally our word for zoo derives from the same origin).

The Circle of Little Animals

To the ancient Greeks this was indeed a circle of little animals, featuring: a ram, Ares; a bull, Taurus; Pisces the Fish; and many other well known (for all the wrong reasons) constellations. It also features three humans: Aquarius the Water Carrier, said to represent Ganymede, beloved of Zeus; and Gemini the Twins, Castor and Pollux.

The only zodiac constellation which is inanimate is Libra the Scales, taken from Babylonian astrology. The Greeks however didn’t recognise Libra; instead they thought that the stars here marked out Scorpius’ claws, which they considered to be a separate sign.

So the twelve constellations that lie along the ecliptic are most well-known due to astrology, a pseudo-science that suggests there is some significance to which constellation the Sun was in when you were born. This is, of course, bullshit.

There are so many reasons why astrology should be laughed off as pre-scientific magical thinking (no evidence, no mechanism by which it might work, inconsistent etc) but next time you meet an astrologer ask them what star sign you would be if you were born between 30 November and 18 December. If they tell you Sagittarius (if they’re a Hindu astrologer they might also say Scorpius) then tell them they are plain wrong.

On these 18.4 days of the year the Sun is wonderfully absent from the usual twelve zodiac signs, It is still there, however, gracefully moving along the ecliptic, but between 30 November and 18 December it is in the constellation of Ophiuchus the Serpent-bearer.

Ophiuchus does not appear in any astrologer’s zodiac. Back in the early days of astrology, when it was first dreamed up several thousand years ago, there were indeed only twelve constellations lying along the zodiac. Over the past few millennia however the Earth’s axis has wobbled slightly (an effect called precession) with the result that the line of the ecliptic has moved with respect to the constellations, and so an interloper, Ophiuchus, has crept in.

So celebrate all those of you born between 30 November and 18 December (one person in twenty share this star sign); you’re not a Sagittarian at all; you’re an Ophiuchan.

It’s still all bullshit though.

* the Sun, of course, does not orbit the Earth, it’s the other way around. It just looks like it does from down here…


Awards [Blush]

November 8, 2010 Leave a comment

This year I was fortunate enough to be the recipient if two fantastic astronomy awards, and a nominee for another.

In April 2010 I was nominated for the UK Space Conference’s Arthur Clarke Award for Public Promotion of Space (it was won by EADS Astrium).

Then last month, while speaking at the Federation of Astronomical Societies’ 2010 Convention, I was presented with two awards:

The 2010 Eric Zucker Award for Outstanding Contribution to Astronomy, awarded by the Federation of Astronomical Societies


The 2010 Joy Grifiths Award for Meritorious Efforts in the Cause of Darker Skies, awarded by the British Astronomical Association’s Campaign for Dark Skies

Needless to say I was chuffed to win these awards, and they have pride of place on my workdesk:

My Awards!

Summer Hiatus

November 8, 2010 Leave a comment

It’s been exactly five months since my last post, due to a combination of factors: Sam went back to work after maternity leave, and I dropped my workload to 2.5 days a week to help with childcare; I went freelance on top of the end of my last contract; and the lack of dark skies over the Summer meant a drop in my astronomy output!

Normal blogging will hopefully resume as of now!

Categories: Other stuff
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