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The amazing run of clear nights continues combined with being at home every night means that I have imaged this comet on 7 consecutive nights now. This early stack tonight is an weak unsharp mask on the coma region showing the various components. The one to the top right (NW) is probably the residual nucleus.
Absolutely sure. This is a sigma-clip stack tracked on the comet’s motion. Stars will be faint streaks. Also this appears on multiple stacks always in the same position relative to the comet. And loads of other observers have imaged it…
This image from tonight is at an image scale of 1″.29 per pixel with FWHM = 2″.9. It is an average stack of 57x60s frames with local flux subtracted using a 6×6 median. It is upsampled by a factor of 4 for display. There is a clear condensation to the NW of the bright extended coma. Interestingly, if you do astrometry on this condensation you get a position which is within 2 arcsec of the position predicted by the orbit using astrometry up to March 25. Current astrometry which is centroided on the bright elliptical coma is off by around 11 arcsec now. This condensation wasn’t visible in my images last night.
Is it what remains of the nucleus? We’ll find out over the next few days.
That is very interesting, particularly the continuing strong C2 emission line. We now seem to have a cloud of rubble moving down the tail but the total magnitude is also falling which would imply that there was no sudden release of gas into the coma at the breakup. This implies that the comet had pretty much exhausted its volatiles before it broke up so we should now see the outer come fade and dissipate since it has no source at the centre. It would be good to follow this spectroscopically as long as you can.
Yes, I’m afraid C/2019 Y4 (ATLAS) looks as if it will soon be an ex-comet. Only a week ago I gave our first webinar talking about prospects for this object. Now I think it is probably a cloud of rubble. As Comet section Director I’m not having much luck with comets!
In my images over the last few nights I have not seen any fragments in the tail. What I have seen is a gradual reduction in the peak pixel ADU count and a flattening/broadening of the downtail coma brightness profile. This plot shows a cut through the photocentre aligned on the tail PA (positive offsets are tailward) for five nights from March 25 to April 7. You can see that peak pixel ADU falls from around 8000 to 1200 in that time (a fade of around 2 magnitudes) and the profile is broader with a more gradual tailward slope in the later images. It looks to me as if the nucleus has completely fragmented and what we are seeing is a cloud of rubble migrating down the tail. This explains the large astrometric residuals in RA since the photometric centroid is no longer aligned with the original nucleus.
If this is correct the future of this comet is as a fainter and fainter diffuse rubble pile. Let’s see what happens and keep this under observation as long as possible. We have a ringside seat to watch the distruction of a Solar System object.
Great memories and I’m already looking forward to next year when hopefully things will be back to normal. I’ll really miss it this year though. Such a shame given all the effort that Ann and Alan and others put into arranging it.
Perhaps we should set up a virtual meeting in the bar on Saturday night. I have plenty of beer since my local brewery is making home deliveries and I’m trying to keep it in business.
Mine from Chelmsford is here (attached in full res). It was taken at 19:32 since clouds were coming in. I have a less overexposed one if that helps. I do have an image at 19:52 which is the closest to 8pm I have.
I’ve just added another video from John. This one is about observing the ISS. Go you our Youtube channel to watch it.
Try the two comets C/2017 T2 and C/2019 Y4. They are both well placed and around mag 8. I know that they are fuzzy and that they move but I’m sure that go-to mount will find them!
It is definitely worth a trawl around the Section pages. There is loads of interesting stuff to read on this site. The old Lunar Section publications are definitely worth a read, particularly if you knew or know of some of the characters therein. Can I also put in a plug for the old Comet Section circulars to from 1973 onwards. They are here.
Yes, me too on my meteor cameras. The number of aircraft in the south east of England is falling rapidly. A very small positive amongst a sea of negative. It looks as if we will have several months of this.
If they cross Denis I would be really worried since the spaceport is on the north coast and they will be aiming north on the one day a year that it is calm enough to launch…
At least the next 60 have been delayed a bit by today’s Falcon 9 post-start launch abort. So far I’ve not found the trails troublesome on my meteor cameras. The satellite motion is too slow to trigger them and I only pick of the trails if something else does. Denis, I know it is not a problem where you are but I have many more problems with aircraft trails. I guess that problem might decrease a bit over the next few weeks.
Certainly if there is no confirmation from another camera this would be the most likely cause. I get quite a lot of nocturnal birds/bats on mine illuminated by streetlights but they don’t tend to fly in straight lines.
That’s an impressive capture. I’ve seen many examples of dual, and even triple, meteors with the same radiant on my video but never anything quite like this where there are two objects so close. It was clear here last night and my NW cam points in your direction but I didn’t pick anything up at that time.
I’m playing around with RMS using a Pi4 and a cheap IP camera but haven’t had much time to sort out the various problems that have arisen so still rely on the old UFO Capture/902H2 setup.
Nice stamps. That plural is certainly correct in the original latin (where they had strict rules about such things) but I doubt if many Engish speakers would use it now. Reminds me of the Romanes eunt domus skit in the Life of Brian…
That would be a sad end for IRAS (famous for the discovery of C/1983 H1 Iras-Araki-Alcock). The predicted time of close approach is 23:39:35 UTC tonight according to LeoLabs.
