Posts Tagged ‘Extrasolar Planet’

Spectrum

What do you do when the weather has been foul and you haven’t been able to do any kind of observing or imaging for a good few days? You build a spectroscope of course!

In all seriousness, the weather has been pretty dire here. Just infinite miles of grey cloud and rain. How do I manage to stay optimistic!!? Anyway, with little more to do than stare blankly at the monolithic cloud cover I thought I’d undertake a little science project. I discovered a nice tutorial for creating a simple spectroscope over at Orbiting Frog and thought I’d give it a go.

As you can see from my attempt, it’s not exactly cutting edge technology but it does the job. I might add, that I omitted the razor blades from my spectroscope purely because I didn’t have any to hand. The end results probably aren’t as focused as they could be if I had used razor blades, but it works, and that’s the main thing.

So how did my homebrew spectroscope fair then? Just take a look at a couple of shots that I took using my Pentax Optio S50 DSC.

On the left hand side you can see light from a dull, overcast day split into it’s blue, green and red components as it passes through the spectroscope while on the right, light from an 11 Watt energy saving light bulb is split. These two light sources produced similar results that are also slightly different. The spectrum from the daylight is diffuse and merged while the spectrum from the light bulb is spread out more with gaps between the blue, green and red.

Compared to the equipment that the professionals use my spectroscope brings new definition to the meaning of low grade, but it gives a pretty good idea how scientist can use one to analyse the chemical composition of stars, nebulae and planets whilst also aiding in the discovery of extrasolar planets.

This really is a worth while and fun project that I’d recommend you try if you’ve got some free time on your hands. Now all I’ve got to do is think about how I can make a larger more permanent version of this kind of spectroscope.

Catching Photons

The sky early on Sunday morning (05.10.08) was the best I have seen in a long while. The Astroforecast Dot Org put sky transparency at about average but from where I was observing at 02:30 UT it looked a lot better than that. This wasn’t one of my usual sessions, instead it was a great chance to take my shiny new Sony a200 DSLR for a test drive, and believe me, I had no illusions that there were going to be dud shots a plenty and a lot of experimenting going on.

It’s one thing reading up on f/stops, focal length, ISOs and exposures . . . it’s another putting it all into practice. I thought I’d take small steps and start things off by trying my hand at photographing constellations. First on the agenda was Cygnus. Focusing on infinity proved to be a real pain in the neck and I probably should have had the foresight to set the focus ring on the 18mm - 70mm zoom lens earlier in the evening.

Captures were predictably awful, but I persevered. I was pleasantly surprised when I spotted Orion just rising over the roof tops to the south east at 02.44 UT. I quickly positioned the tripod and the camera and began shooting. I started off at f4.5 using ISO 800 and a 5 second exposure. I then upped this to 10 seconds and then finally 30 seconds. It was the 30 second exposure that won the day and offered up the best (albeit slightly out of focus) capture of the evening revealing both M42 (The Orion Nebula) and M43 (De Mairan’s Nebula) as well as the star Iota Orionis which forms the tip of Orion’s sword.

I returned to my original quarry of the evening - Cygnus, which was now sinking slowly towards the horizon. Using an f/stop of 3.5 and a focal length of 18mm I managed to capture this  30 second exposure at ISO 800. Not the most dramatic shot, but it’s early days. Like the Orion shot, light pollution was quite visible in this capture as was some chroma noise, but I managed to process the worst of it out in Photoshop. I should have had the foresight to take some dark frames (note to self: TAKE DARK FRAMES!).

The white giant Deneb can be clearly seen while the star fields and dust lanes of the Milky Way are just visible as they tumble down the length of Cygnus. The top of Lyra can be seen drifting slowly out of view while Vega1 hovers just above the roof tops. Over to the far right of the image can be seen the constellation Draco or as the ancient Egyptians called it Taweret which means one who is great after the goddess of the northern sky.

By about 03:20 UT the cold really was beginning to set in so I decided to put the DSLR aside, but before I called it a night I decide to do a little observing through the Bresser 10×50s. Turning the binoculars on to Orion, I took a look at M42 and what a view - just stunning. Randomly sweeping the sky, I eventually landed on Ursa Major and took a peek at The Horse and Rider i.e. the stars Mizar and Alcor. Turning towards the zenith I decided to take in another view of M31 before sweeping south on to The Pleiades and finally back to M42 in Orion.

All in all, I’m quite pleased with my first proper attempts at DSLR astrophotography but I’m sure I’ve got a long way to go yet before reaching the next level.


  1. Based upon excess emissions of infrared radiation coming from Vega, it was ascertained that there was a disk of dust around the star much like the Kupier Belt of our own solar system. Irregularities in this disk of dust also suggest that there is at least one planetary body with a mass equal to Jupiter in orbit around the star.

Going Extrasolar

Surprise, surprise . . . clouds and rain, so no observing at all for the past week. To stave off withdrawal symptoms I thought I would post up another Blender render that I produced several weeks ago.

It started by browsing the New World Atlas at the JPL site Planet Quest. 47 Ursae Majoris, a yellow G class star 43 light years from Earth with two planetary companions (47UMb and 47UMc) was a completely random choice on the list. I soon started to wonder what exactly a planetary system around this star would be like. The render above gives an impression of what 47 Ursae Majoris b may look like - a large gas giant discovered in 1996, it has a mass of 2.41 Jupiters and orbital period of 1095 days.

The second known planetary body 47UMc lies 3.73 AU from it’s star and lies a little further out than 47UMb, but that’s a render for another time . . .