Webcam astronomy: simple but effective

Over the past 4 years, I have been steadily assembling equipment for the purpose of photographing deep sky objects (DSOs). These are dim, sometimes large, diffuse cloudy patches when viewed using binoculars or a small telescope. Starting with the Andromeda galaxy (see below), I used a simple, long tube telescope fitted to a tracking mount (that tracks the DSO as it moves across the night sky). This allows a camera to collect light over a long period of time (often up to several hours) showing features that would otherwise be far too dim to detect with the naked eye.

The Andromeda galaxy (M31) taken by collecting over 2 hours of photographic exposures.
The Andromeda galaxy (M31) taken by collecting over 2 hours of photographic exposures.

Although I personally find this type of astrophotography very rewarding, there are some major drawbacks. The first and most severe is how sensitive this type of photography is to unwanted light. Since photographing DSOs requires a really long exposure, any stray light from streetlights or the Moon simply washes out the object’s detail. The second is the sheer time it takes to collect the light to produce these types of photographs. The main issue is that as I take these long exposures (typically I take over 30 shots each lasting up to 5 minutes), any disturbance such as a gust of wind or nearby movement can cause the image to smear.

Mainly for these two reasons, I decided recently to branch into a different type of astrophotography – webcam astrophotography. Although I don’t have any pictures to show yet (I haven’t finished modifying the webcam yet, but watch this space!) I will briefly discuss the principles of this form of astrophotography and how it can be achieved with very limited equipment (and budget).

Put simply, webcam astrophotography involves taking a video of a bright night sky object (such as a planet or the Moon) and using the best frames of that video to produce a high quality image. There are several advantages to this approach. Firstly, since the object you are photographing will be bright, the exposures are short. This means that movement of the telescope will not cause image smear. In addition, the telescope mount does not have to track the night sky very accurately since each frame of the video is taken over a fraction of a second (normally 1/30s). Secondly, bright objects far outshine artificial light pollution, which makes this form of astrophotography very suitable for people living in towns and cities.

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Photo of a bird with strong chromatic aberration caused by improperly focused violet light.

So, with a webcam and a cheap telescope mount, some impressive   astrophotography can be achieved (see this link). However, I have neglected to mention anything about the telescope. When photographing bright objects overcoming chromatic aberration (CA) is a real problem. This optical aberration occurs when light being focused through a lens splits into its constituent colours and these colours focus at different points. The colour fringing effect caused by CA is shown on the right.

So, I decided t20160130_093248o use a telescope design known as a Maksutov-Cassegrain (modelled by my lovely fiancée Sarah) that avoids CA through an ingenious use of lenses and mirrors. There are three important advantages of using this telescope. (1) The light entering the telescope does not split into different colours (as mentioned). (2) Light is also neatly folded up so the actual telescope is conveniently small. Finally, although the telescope is short, it is capable of imaging at high magnification – an important feature if you wish to image small Moon craters or the great red spot on Jupiter.

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A excellent image of Jupiter taken using a Maksutov-Cassegrain telescope and a cheap webcam. Photo credit: Dion from the Astronomy Shed.

In hindsight, perhaps I should have started my astrophotography hobby with webcam imaging; I would have saved a lot of time and money and not developed an irrational hatred of streetlights or the Moon!

Post by: Daniel Elijah

The astronomy of astrology

It’s been a while since I last posted so instead of talking about the details of using telescopes or taking astrophotographs, I will discuss what for many people are two interchangeable terms: astronomy and astrology. More specifically, this post shows how some interesting oddities of astrology can also interest astronomers.

As a reminder, astrology is the study of the movements of celestial objects with the goal of predicting or justifying life events while astronomy is the scientific study of the properties, interactions and evolution of celestial objects. While I feel that our life choices are not influenced by the movement of the Sun across the zodiac constellations, or the alignment of certain planets I do think that people who believe in astrology may find significant interest in the evidence-based view of the universe astronomers take.

Lets begin by discussing an interesting tenet of astrology: star signs. The 12 signs of the western zodiac are based on the constellations which lay along the path on which the Sun appears to travel over the course of a year. Your star sign should ideally relate to the constellation which the Sun passes through on the day of your birth. But, most the time things are not this simple.

Every year, as the Earth orbits the Sun, the line of sight between us and one zodiac constellation is blocked by the Sun, this means that, as viewed from Earth, the Sun will appear to be sitting within this constellation. However, the dates associated with the star signs have not been technically correct for around 2000 years, i.e. the constellation in which the Sun appears the day of your birth may not fit with your star sign.

This is caused by a discrepancy between the way we define a year and changes in the movement of the Earth. As a society, we define a year as starting on a set date (the 1st of January) and running for a given number of days (365 – or 366 on a leap year). However, a year in astronomical terms is defined as the time it takes for the Earth to revolve once around the Sun, and these two measurements do not necessarily match up.

Figure 1. The position of the vernal equinox in the night sky. The Sun currently passes through this point on the ecliptic (red line) on 20th March. Graphic taken from Stellarium.
Figure 1. The position of the vernal equinox in the night sky. The Sun currently passes through this point on the ecliptic (red line) on 20th March. Graphic taken from Stellarium.

Specifically, in astronomical terms a year consists of the time period between vernal equinoxes. The vernal equinox occurs when the ecliptic (the line the Sun makes across the sky in one year) crosses the celestial equator (an imaginary line projecting out from Earth’s equator into space), see the blue arrow in Figure 1.

However, due to the fact that the Earth slowly wobbles on its axis every 26000 years (called Precession), the date of the vernal equinox slowly shifts by about 1 day every 70 years. The effect of this shifting equinox is that the position of the Sun within different constellations slowly changes, therefore, the Sun may be in a different constellation during the month of your birth than it was when astrological charts were first drawn up. Below is a table comparing traditional star sign dates with the actual position of the sun on these dates.

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The table also includes the length of time the Sun spends in each constellation. As a convenience in astrology, the star signs are given equal lengths. However, in reality, constellations have different sizes and cut across the ecliptic at different angles. The Sun spends 44 days in the constellation Virgo but only 8 days in Scopius (making true solar Scorpios a rare breed!). You may also notice an unfamiliar constellation: Ophiuchus (the serpent barer), it’s a large constellation but only a small part of it is actually crossed by the Sun in early December. Strangely this was known in ancient times but not included as a sign of the zodiac.

Gemini - 2015 Gemini - 28015Figure 2. The motion of the stars over thousands of years changes the constellations. Nearby stars (such as Pollux) appear to move faster. Graphic taken from Stellarium.
Gemini – 2015
Gemini – 28015Figure 2. The motion of the stars over thousands of years changes the constellations. Nearby stars (such as Pollux) appear to move faster. Graphic taken from Stellarium.

So when will the traditional star sign dates once again match up with the position of the sun within these constellations? Well, this could happen in about 24000 years, after the Earth has completed a full precession rotation. However, by then the stars themselves will have moved relative to each other, changing the shape of the constellations forever. In Figure 2, the constellation Gemini (my true solar star sign) is shown as it appears now (2015), and how it is projected to appear after 26000 years of star movement (date 26000 + 2015).

All of this serves as a reminder that the universe does not neatly fit into equally spaced constellations or fixed calendars, instead it is amazingly complex and constantly changing. So perhaps astrology can be a starting point for peoples’ interest in the universe, or at least to getting a better understanding of the science behind the horoscopes.

Post by Daniel Elijah

Shooting the stars – Astrophotography as a hobby

About three years ago, I began to crave a hobby that would satisfy my curiosity about nature but not involve frontline scientific research (my day job). That hobby turned out to be astrophotography, an activity that is both fascinating and challenging regardless of how advanced you become.

After months of comparing different telescopes online, I finally settled on a medium-sized (120mm) refractor (containing a lens at the front), it being simple to use, tough and versatile. I quickly realised that there are many ‘amateur’ astronomers out there who are willing to spend thousands of pounds on equipment, often having multiple telescopes. I however, decided to perfect the use of a modest telescope with the hope of producing pictures that would only be expected from far more expensive kit.

After setting up my telescope and taking a whole array of different pictures, I found my interest moving towards deep sky objects (DSO). These are celestial objects outside our solar system such as galaxies and star clusters. They are normally very dim (often invisible to the naked eye) but, unlike planets, their apparent size (the size they appear from Earth) is typically large. By adding motors to my telescope, I can track these objects as they move across the sky. This allows me to take long-exposure photographs (10 minutes or more) revealing dim structure and colour which is not visible through the eyepiece during normal viewing.

However, I soon realised that my telescope had only limited accuracy when tracking DSOs. This caused DSOs to drift across the camera over several minutes, leaving ugly streaks of light on my pictures. So, my next upgrade was to add a guider; a device that monitors the movement of stars across the camera and sends a correcting signal to the telescope motors if alignment strays. This upgrade means that I can now get clean pictures that show DSOs in great detail – although the guider still needs a bit more work to avoid over-correction.

The pictures below show the culmination of years of small upgrades to my modest telescope. The first shows the Whirlpool galaxy (M51) while the second shows the great globular cluster in Hercules (M13), if you look carefully you may even spot some smaller galaxies lurking amongst the stars (these can be seen as small grey ‘smudges’).

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Whirlpool galaxy (M51) – a galaxy in the process of colliding with a smaller galaxy.
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The great globular cluster in Hercules (M13), a cluster of stars attracted together by their combined gravity.

Post by: Dr. Daniel Elijah.

Note: images were taken from the Galloway Astronomy Center in Scotland (one of the UK’s best dark sky sites)