I’ve always had an interest in astronomy and have dabbled in astrophotography since I got my first digital camera back in the late 1990s. Over the years I’ve got images of all the planets except Neptune and Pluto. The latter of these is never going to be an easy target for the lazy amateur (me), but maybe, just maybe Neptune is possible.
I’ve had a soft spot for Neptune since the Voyager 2 flyby in 1989 – I’ve still got the article I tore out from a newspaper at the time.
As it happens, Neptune is nicely placed in the sky right now – just between Venus and Mars and close to a couple of guide stars.
Braving the frost, I took the camera out to the garden, mounted it on a slightly wobbly tripod and took some images of the general area of sky I knew Neptune was lurking. Some processing and stacking with ImageJ and I had a star-field that might contain my target.
It’s easier to see the faint points of light of the guide stars and Neptune if you invert the colours, so you’re seeing black points on a white / grey background.
I used Stellarium to predict the current positions of Mars, Neptune and the guide stars and overlaid that on top of my image stack. This lined up reasonably well, there are some angular offset and slight scale differences between the two images, but it’s close enough for guidance.
With the assurance that I had Neptune in my images I was able to definitely pick it out from the stellar background.
Sometimes when you’re looking around for something to scan in your new-ish CT scanner the answer just lands in your lap.
I’ve been doing #xraymyadvent again this year, but thought I’d test out the new scanner with an item more in keeping with the scanner’s intended use. Searching around the lab I found no obvious items. Until I looked down at the floor, this is what I found.
A poor dead mouse.
This is just 60 projections from the full CT scan – it looks like the scanner worked well.
Back from having spent a few days between Christmas and New Year in Palma, Majorca. On the last day there I noticed I could just see the dome of the Planetarium of Majorca (or the telescope dome, I’m not sure which) from the hotel terrace. Seeing conditions were not great, but the small white point on the mountain top was clearly visible by reflected sunlight. It did look to be just on the edge of visibility, so now I’m back I wondered just how close to being invisible it really was.
Telescope dome position : 39.642528°N 2.950516°E (from wikipedia)
My viewing position : 39.555666°N 2.623219°E (from photographic GPS and google maps)
Some derived data:
Dome diameter : 15m (measured off google earth)
Distance between these points : 29.668km
Angular size :
1′ 44.3″ arc seconds
This seems pretty small, how’s it compare to things we’d usually see?
Sun diameter : 31’30″Full Moon diameter : 29’20”
Planet Venus at closest : 1’00”
Brightest star in the sky – Sirius : 0.005936″
(All values from wikipedia)
The dome appears larger than the brightest star in the sky and roughly the same size the planet Venus does. These are both perfectly visible, so why did the dome appear just visible to me? I’m guessing it’s because the dome was only reflecting a small amount of light, and I was viewing it against quite a bright background (blue sky) too. Atmospheric haze and thermal twinkles probably didn’t help.
So although I should have been able to see it pretty clearly (if it had been emitting it’s own light, against a dark background) , I was probably pretty lucky to have seen it at all given the atmospheric conditions.
Some time back, a friend @codfishcatfish was building a GPS disciplined oscillator for radio measurements. Part of the circuit uses a MAX232 device to interface the low voltage digital signals to a PC serial port. He found his cheap (from eBay) MAX232s got very hot and failed in use.
It was obvious the devices were fake, so I offered to tear one down to see what it really was, a cheap clone or a re-badged something else?
The standard technique to remove all the epoxy and metal to leave the bare silicon die is to use strong nitric acid. So I cut the legs off the chips, no point wasting acid dissolving those, and ground away some of the epoxy resin to speed up the dissolution.
Soaking the ICs for an hour in room temperature nitric acid had no discernible effect, so I heated up the acid. The reaction became very vigorous!
It took about 20 minutes to remove sufficient epoxy to see the silicon die – it also removed the lead-frame and bond-wires so there was no chance to test the ICs after de-capping.
The ICs were dried and the die removed by scraping away the carbonised epoxy with a scalpel. This done, the die could be examined under high magnification to see if it looked anything like a real MAX232 or I could see any other identifying features.
Comparison with a real MAX232 die proves these ICs are fake. The only identification I could find on the die is the following
So I’m non the wiser as to who actually made these, but the device does seem to show a general resemblance to the layout of a real MAX232 – they didn’t just program a micro-controller to do the job or something similar.
It was just a fun diversion and a chance to try something I’d wanted to do for a while. I might try to find some more interesting ICs to pull apart and take better images of.
Can you really be an eclipse chaser if you’ve only actually chased one eclipse?
My chased eclipse was August 1999 – south west England. Back in the mid 1980s I had a book of fascinating astronomical facts, it listed the dates of upcoming eclipses until the far-off Year 2000. I decided that I’d see that one, and as time passed, I did find myself watching very cloudy skies from a side road near the hurlers stone circle. The sky did darken at the appointed time, the surrounding fields lit up with camera flashes and there was a genteel sense of disappointment when the sky cleared for a glorious sunny afternoon shortly after the end of the eclipse.
I’ve since caught a few other eclipses visible from London, but I’d not gone out of my way to travel to see any. I’ll not count the North American October 2014 partial eclipse as chasing because I was already in the country for other reasons.
Of course it was cloudy for the big event today. My preparation of solar film, pinholes and time-lapse camera was for nothing. With about ten minutes until first contact between sun and moon, I decided I’d at least have a try at logging the change in light levels.
I quickly bodged together an Arduino, an SD card and a light sensor, and put it in the garden. The plan being the thick cloud cover may stop be seeing the ellipse directly, but would act as a perfect diffuser for making whole-sky light level measurements.
The graph shows the result – it got dark(er) when it should have.
The y-axis units should be Lux, but are uncalibrated.
Other eclipses during my life.
July 1982 – No memory of this one. December 1982 – No memory of this one either. May 1984 – Vague memory of my Grandfather trying to view this though smoked glass. May 1994 – Watched this though a pinhole in card held up to my eye. October 1996 – I must have watched this, but I can’t recall it. August 1999 – The big one, had planned to watch this since the mid 1980s. Got stuck in traffic close to our chosen viewing spot (along with half of Cornwall and the BBC), watched from the side of the road. Cloudy, but magic. May 2003 – Far too early for me. October 2005 – Set up with telescope and camera at work, clouds rolled in. Managed to get the occasional glimpse of the sun in projection though the telescope. March 2006 – May have tried to watch this one, but it was only a tiny fraction partial eclipse and I was deep in PhD writing up, so no memory of this eclipse. August 2008 – Another tiny fraction partial eclipse, I think I tried to spot it using a stack of CDs as a solar filter. January 2011 – Early and cloudy, nothing seen. October 2014 – Nicely visible from a front porch in Minneapolis March 2015 – as above, cloudy but at least some data from the eclipse.