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Nick JamesParticipant
Paul,
That’s a nice image. I had a similar view in the early evening. It really does demonstrate how much fainter Jupiter is compared to venus. Here’s my picture from last night.
Nick.
Nick JamesParticipantI did, but visual observing is so hard compared to imaging!
I only have a C6 for visual use mounted on a Vixen Sphinx mount. It found the field without problems and I used around x150 but the conditions were so grotty that I could only see down to mag 12.5 or so (I could clearly see AAVSO star 111 but star 125 was right on the limit). I started to observe around 2240 UT and initially I couldn’t see V404 Cyg. It then gradually became visible until around 2320 when it disappeared over a period of a few minutes even though stars of similar brightness were still there. Ten minutes later it was back and brightening but I had to go to bed…
I must admit it was very nice to see photons from a black hole jet with my own eyes but it made me realise how good CCDs are for imaging things in light-polluted places!
Nick
Nick JamesParticipantI’ve been doing an Ic Band run on V404 Cyg tonight with 30s exposures. The conditions are dreadful with drifting cloud and haze but the star is currently varying rapidly. It has just dropped from Ic=9.7 to Ic=11.6 in 12 minutes!
Nick JamesParticipantI did another run of 4 hrs last night and V404 Cyg was at around Ic=10.2 with variation of around 0.3 mags. We seem to be getting the boring bit of the lightcurve at our longitudes as you can see from the attached AAVSO Ic lightcurve. My observations are the ones in blue.
It’s definitely worth keeping this object under close observation.
Nick JamesParticipantIt got a bit more interesting later in the night.
Nick JamesParticipantI’m observing V404 Cyg again tonight this time using 30s exposures in Ic. The lightcurve so far tonight is attached. The mean Ic mag is around 10.4 and there are variations of a few tenths of a mag. Nothing like as spectacular as a few nights ago.
Nick JamesParticipantRichard,
The McDonald data is very nice. It shows what can be done with a 2.1m telescope and a specially designed photometer running with a 2s cadence. The Argos photometer is described here.
Nick JamesParticipantI managed a very short run of less than an hour last night in a short clear patch. There was a lot of variation (> 1 mag). Peak mags were 9.8 in Ic, 11.8 in V.
Nick JamesParticipantHere’s the updated lightcurve covering the whole of last night.
Nick JamesParticipantMichael,
I’ve never seen an eclipse from an aircraft but it clearly gives a completely different perspective on the various wide-angle phenomena, particularly the shadow. Thanks for posting these images. It looks like you had clear windows. I know that some of the eclipse flights had real problems with ice on the windows.
Nick.
Nick JamesParticipantJust listened to it. It sounded like a radio adaptation of the early part of Martin’s book with several of the facts changed for dramatic effect. I liked the quote “Does anybody actually read the BAA Journal?”. It’s not every day that you get something like that on Radio 4!
Nick JamesParticipantAnd he did a very good Radio 4 adaptation of Steven Baxter’s alternative history of the Apollo programme, Voyage. I’ve set my recorder for Monday afternoon.
Nick JamesParticipantCouncil on Wednesday agreed that the BAA should produce a DVD of this eclipse. This will include video and stills of the total and partial. We would particularly like to have material from groups around the country who set up public events to observe the partial.
I’ll make a more detailed announcement shortly which will include details of how to submit material.
Nick.
Nick JamesParticipantMike,
That’s a great interview. Do you think they worked out the acronym for your travel group’s name? Remind me to get an autograph next time we meet!
I agree that the shadow bands were very prominent. I did help that there was a very large expanse of white “sheet” to see them on but I’m sure that the very clear atmospheric conditions helped too.
Nick.
Nick JamesParticipantThanks Grant and Gary. It does seem that it was rather hit and miss in the UK but many people saw it.
I’ve just watched my recording of the BBC’s Stargazing Live coverage. I wonder if I can charge them for the cleaning bills that resulted from me throwing stuff at the TV. It seems to me that it would be a good idea for the BBC to actually have someone who knows something about what you see during a total eclipse so they can explain it to the audience rather than having celebs sprouting total nonsense. Perhaps that is too radical an idea?
I’ve spent the day processing my video and stills. Here are some links to stills and video captured in Svalbard on Friday. I apologise for the commentary on the video. It was -21C or so and my brain had died. I do get the impression that the eclipse was “incredible” or “amazing” though.
Nick.
Nick JamesParticipantDavid,
I think it has been suspended for a month while Stargazing Live is on. It’s due back in April.
Nick.
Nick JamesParticipantStan,
The key point is that any filter must go over the front end, or objective, of the telescope. It is not safe to use filters at the backend, i.e. near the eyepiece.
I have a C6 and observe the sun using a full-aperture filter made from Baader Solar film. You can buy this film from a number of UK suppliers and make it into a filter that fits over the objective of your telescope. I made a suitable filter using cardboard and tape as shown in the picture below. Make sure that this fits snugly over the objective so that there is no danger of it coming off when you are looking through the scope.
Let me know if you need any more info.
Nick.
9 February 2015 at 10:46 pm in reply to: Potential visibility of a fuel dump from a rocket booster #576792Nick JamesParticipantWilliam,
Michael’s pics are excellent. Seeing it in a wide field really shows how bright it was. I wish I’d seen it!
Nick.
Nick JamesParticipantMike,
I think the adopted rotation period is 2.6 hrs with a lightcure amplitude of around 0.2 mags. That means that I should have two rotations on the image set that I took on close approach night but I haven’t managed to find the time to do the initial analysis yet. Richard Miles has been helping me with the details and we hope to have something soon. The lightcurve may even show the effects of the small moon. Keep an eye on the ARPS page for more info.
You’re right that the motion was fast but the asteroid was so bright it was detectable with small instruments. Most of my images were made using a 72mm f/6 WO Megrez refractor and CCD tracked at sidereal rate. The wide field makes photometric reduction easier since there are lots of suitable reference stars visible.
Nick.
Nick JamesParticipantIt’s still visible tonight around 12th mag and moving much more slowly.
Nick
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