Photometry

This is a brief summary of my early attempts at measuring the light curves for short period binary stars.  My initial attempt has been sort of a proof of concept using Algol as a target.

Objective:
Produce a light curve of the minimum of the transit of Algol

Equipment:

• Canon xTi
• Standard photography tripod
• Canon remote timer

Method:

During the late fall and winter Algol is in an excellent location in the sky for photography. To complete the light curve analysis I'm looking for its not actually necessary to photograph the entire period of the binaries rotation; photographing the length of the minimum is the primary goal.  Fortunately for me Algol has been well studied and the time of the minimum on any given day is available on the Sky and Telescope website:

Sky & Telescope Algol Minimum Calculator

The Algol binary system has a period of 2.8 days and the transit of Algol b takes 10 hours from start to finish.  Ideally this entire transit is what should be photographed.  However this requires 10 hours of clear dark skies during which the minimum occurs.  This is rare and so far I haven't been able to photograph more than a few hours at a time.

Results:

This past weekend I attended the Alberta Science Teachers Conference in Banff and Thursday November 15th at 11:56 pm was a predicted minimum of Algol.  So after the conference ended I set up my camera and recorded about an hour of photos immediately up to the minimum.  After gathering twenty seven 20 second pictures at three minute intervals I converted the .raw files to .tiff files using photoshop.  I was able to analyze these images using SalsaJ and came up with some encouraging data.

Below is a quick time lapse of the images I took.  Some of the pictures were effectively ruined by transient clouds but enough suitable images were obtained to provide a rudimentary proof of concept. 

Using the best 7 data points I was able to using the photometry features of SalsaJ to gather the data below:

 

Image #	Start Time	Target Intensity	Comparison Intensity	Magnitude Ratio
1	21:53:00.00	3519840	4879236	0.72139
2	22:55:00.00	3402002	4836478	0.70340
3	22:57:00.00	3819125	5215910	0.73221
4	22:59:00.00	3773813	5597030	0.67425
5	23:01:00.00	3691644	5714231	0.64604
6	23:03:00.00	3980940	6143964	0.64794
7
8
9
10
11
12
13
14
15	23:27:00	2907813	4760742	0.61079
16
17	23:33:00	3614116	6708249	0.53876

For the photometric analysis the comparison star was Mirfak. Using the ratio of Mirfak to Algol during the image run I created the light curve:

Analysis:

These results are encouraging. Even though the weather resulted in a large gap in the data and there are relatively few points, they consistently show a decrease as the expected minimum approaches.   I'm further encouraged because of the specific results of the photometry.  Mirfak is not a variable star and has an apparent magnitude of 1.8. At its minimum Algol has a magnitude of 3.4.  The ratio of magnitudes of Mirfak/Algol at the minimum of Algol is 0.529 which is very close to 0.538. The deviation could easily be explained by the time difference between my last observation (11:33 pm) and the time of the expected minimum (11:54) or the effects of clouds on the observations.

Conclusion:

While this isn't conclusive I'm quite encouraged by my results.  I've been convinced this method will eventually yield successful results when the weather and transit times allow me to make further observations. If you have any suggestions or comments I'd be happy to hear them.

Fall Observing

I've been busy the past 6 weeks. And thankfully much of it has been observing.  Anyway, I'm going to keep this short and simply post a few of the pics I've taken.  More to come on them later.

 

Telescope: Celestron Edge 11"

Mount: Skywatcher EQ6

Camera: Hutech modified Canon T3i

Exposure: 14 x 5 min at 1600 ISO

 

Telescope: Televue 85 mm

Mount: Skywatcher EQ6

Camera: Hutech modified Canon T3i

Exposure: 11 x 5 min at 1600 ISO

 

Telescope: Televue 85 mm

Mount: Skywatcher EQ6

Camera: Hutech modified Canon T3i

Exposure: 13 x 5 min at 1600 ISO

 

Camera: Canon xTi

Mount: Canon camera tripod

Exposures: 65 x 1 min exposures combine using startrails

Deep Sky with the Edge 11"

Its been a busy couple of months.  My wife and I finally moved back to Edmonton and for the past two weeks or so I've been reaping the astronomical benefits.  The skies were ridiculously clear, if not extremely humid.  Dew has been a major problem but not so much as to stop me from Stargazing.  I spent three or four nights out at the Blackfoot Staging Area (its one of the local RASC observing sites) testing the conditions and starting to put my 11" Edge through its paces.  I also got to catch the Perseid meteor shower! What an amazing night.  I brought my wife and several friends with me and in a few hours we saw dozens of meteors, the International Space Station, Jupiter, the Moon, the Milky Way, and about half a dozen deep sky objects.

I also noticed a few other things

1)  My old battery is basically dead.
2) The new site is quite a bit better than the site I had in Vancouver
3) The Edge is an amazing telescope

I'll write a post soon about how I overcame my dead battery because rather than buy a new one I actually built my own astronomical power station.  For now I'm just going to post a few pictures I took from the Blackfoot Staging Area.  There are a few Deep Sky objects like the Dumbbell Nebula and the Iris Nebula along with a wide angle shot. I would have like to do longer exposure but as I mentioned before dew was really becoming a problem.

 

11 x 5 min @ 1600 ISO

 10 x 5 min @ 1600 ISO

2 min exposure with Rebel xTi with 16mm Lens

The last picture was actually a series that I planned to use in a short time lapse.  The object in the foreground is my telescope with the Milky Way in the background.  The bright streak across the sky is the International Space Station. I had intended the time lapse to be quite a bit longer but again, the dew got in the way. So here is the 5 or so seconds of the movie.

Didn't turn out to badly but by the end you can start to see the effects of the dew on the camera lens. Of well, hopefully as we move into the fall dew will be less of a problem.

Sun Spots

The Transit of Venus came and went and much to my extremely disappointment the weather in Vancouver well, disappointed.  The end result was that I missed the Transit.  Nothing but clouds and rain.  Since then the weather has cleared up slightly, which is to say every now and then you can see some patches of blue.  This frustrates me on several because I bought a white light filter for my new 11" telescope that I really haven't been able to use.

Well, today I spotted a break in the clouds and made good use of the brief appearance of the sun.  The first picture shows about a quarter of the solar disk.  In the center of the picture is active region 1504 which contains about half a dozen sun spots.  Below and to the left there are a few more faint sunspots.  Presumably each of these sunspots have some sort of active prominences or flares but we can't see them in white light.  

 

This is a close up of active region 1504 taken through my 11" SCT with a canon T3i using a 2x Barlow.  I would have liked to do a few more high resolution shots but tracking, wind and eventually clouds made than impractical.  Fortunately the sun isn't going anywhere!

The Sun in HA

With the transit of Venus coming up in a few weeks I decided to take my solar telescope out. For those of you who have never heard of Coronado's (now Meade's) Personal Solar Telescope I'd encourage you to check it out.  It runs for about $500 and is one of the cheapest ways to look at the sun in Hydrogen Alpha.  Although it gives a tiny, full disk view of the sun its the easiest way to see solar flares and prominences that aren't visible through a white light filter. 

Anyway, its not designed for imaging because its nearly impossible to get a camera's chip close enough to the focal plane.  However, for anyone interested it is possible to do: you need to add a Barlow lens to your image train.  I actually used a 5x powermate last Sunday and got some absolutely stunning images of flares and prominences.  If your interested in the sun, this is really the best way to look at it without spending thousands of dollars. 

 

One of the things I found most interesting about these pictures was when I compared them to my earlier attempts.  Its nice to know that I'm actually getting more proficient at using my camera and telescopes.

 Not only do the new pictures show more solar detail but they are also taken with larger format camera and almost at a size I could print.

M51

M51 and the new Edge

Over the course of 2 days I spent close to 16 hours on Mount Seymour stargazing.  A significant portion of that was used to image M51 and the M57 to try and test out the optics on my new Edge 11" telescope.  Unfortunately I also noticed that my motorized focuser kicked the bucket so I now either need to repair or replace it; focusing a SCT with the standard mirror control is unbelievably frustrating.  Anyway, M51 presented me with a great opportunity to compare the quality of my old Celestron 8" with my new 11" because just a few months before I imaged M51 with the old scope.  And as an added bonus I even have an image of M51 through my Televeue 85 mm.

The two SCT telescopes imaged M51 for about the same amount of time so the images are pretty easy to compare. 

M51 through Edge 11" - 12 x 5 min

M51 through Celestron 8" - 15 x 3 min

M51 through 85 mm Televue 12 x 3 min

Comparing these shots I'm definitely the most impressed with the Edge, but it is also the scope that needs the most work to use.  Its bigger, which makes it more difficult to set up (and the mount is quite a challenge to physically move when polar aligning).  The longer focal length also means it needs to be better focused, which is why my motor focuser really needs to be fixed.  I'm quite excited about the prospects of continued imaging through it!

The Super Moon

I don't know why but for some reason the media really picked up on the full moon this month.  Because the full moon occurs when the moon is at perigee (its closest point to Earth) its called a 'super moon', but really its not that special.  This particular lunar configuration happens quite often and it would be really difficult to spot the 15% increase in size. I was quite interested in setting up my new telescope (an 11" SCT on a EQ6 mount) and testing it out.  Because I was just working the kinks out of the new setup I didn't really want to drag it all the way up the mountain so I chose a community league parking lot close to my house.  My plan was to take some shots of the moon and then try a Light Pollution Reducing filter and see how things in the city worked out.  Unfortunately I made a little mistake; I never labelled which filter was which in my filter wheel and ended up doing all the imaging through a narrowband OIII filter. Sadly, the result was not good.

The moon however turned out quite nicely!