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I think I detected it using a 90mm refractor from Chelmsford last night:
https://britastro.org/observations/observation.php?id=20250703_210130_832805f398624544
It is right on the limit of detection using a stack of 88x60s frames but I’m pleased to have got it from the UK given that my main telescope can’t get that low.
Nick – Great image.
Here’s mine. I can’t get that far south with my main scope due to a neighbour’s tree. This is from Chile:
https://britastro.org/observations/observation.php?id=20250703_055356_fc54046de537751b
The detection of cometary activity is really exciting. It looks as if this object will be brighter than mag 20 for the next year or so and it will be well placed for us in the northern hemisphere after perihelion. A great opportunity to study something from another star system.
Good luck Nick. Yes, 18.5 should be relatively easy even that low down. I have a tree in that direction that blocks my main telescope so I’ll have to go remote.
Who’s going to be the first person to get an interstellar object with a Seestar?
Nick.
In case anyone needs an ephemeris for the next few days I’ve just generated this from Findorb. It is for Rio Hurtado, Chile but the parallax is small so it will work for anywhere.
The current elements from Findorb using all of the astrometry on the NEOCP are:
<plaintext>Orbital elements: A11pl3Z Perihelion 2025 Oct 29.67795 +/- 0.216 TT = 16:16:14 (JD 2460978.17795) Epoch 2025 Jul 2.0 TT = JDT 2460858.5 Earth MOID: 0.3549 Ju: 0.2479 q 1.34626730 +/- 0.0133 Ma: 0.0201 Sa: 0.4082 Find_Orb H 11.91 G 0.15 Peri. 128.11453 +/- 0.14 z -3.7575161799 +/- 0.0375 Node 322.06864 +/- 0.10 e 6.0586211 +/- 0.1 Incl. 175.10933 +/- 0.0044 111 of 113 observations 2025 June 14-July 2; mean residual 0".37</plaintext>Yes, this is a very interesting object that appears to be brightening quite rapidly so it could be cometary (I hope). We’ll have plenty of time to observe it but not when it is at perihelion since it is at inferior conjunction then. I’m preparing a news note and will upload it later. Astrometry will be very useful but the arc (with precoveries) is already long enough to give us a pretty stable orbit solution. It is definitely interstellar with a rather high approach velocity.
For now, beware the most planetarium programs will break with elements that have e=6!
Here’s a link to the real-time video clip from UK004E. The cloud starts in northern Capricornus and then moves up into Aquila. You can see a number of the deployed spacecraft ahead of the cloud and a brighter object in the cloud. The brightest dot, towards the end, is the venting second stage itself. Mel’s video linked above shows the individual events in far higher resolution and I assume that the significant brightening of the second stage around 00:12:45 is the large venting event shown on Mel’s video.
https://nickdjames.com/Spacecraft/20250524_propvent/UK004E_20250624_001126_ndj.mp4
The final spacecraft deployment was the Mission Possible re-entry experiment at T+2:43:53 which is just before 00:09 UTC and the first sign of the cloud is at around 00:11:30 so only around 2.5 mins later.
Stan,
According to the Space-X video here:
https://www.spacex.com/launches/mission/?missionId=transporter14
The second stage de-orbit burn occurred over north Africa starting at T+2:40:16 and it lasted a few seconds. Launch was at 21:25:00 UTC so that means that the burn was over by 00:06 UTC, before we saw the stage come over the UK. Three minutes later it deployed a re-entry demonstrator called Mission Possible and then started the passivation with thruster firings and venting residual propellant which is what we saw.
I have video from my SE pointing camera (UK004E) showing the stage rising out of the Earth’s shadow in the SSE with with the venting starting around 00:11:46 UTC.
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Mel – That’s a brilliant video and it shows the various thruster pulses and the main burn very well. What equipment did you use?
Steve – You were in bed? So was I. I thought you had an army of Seestars permanently monitoring the sky…
Cees Bassa confirms that it was Transporter 14. Presumably the upper stage deorbit and passivation.
I don’t yet know what it was but it certainly looks like propellant venting. Prompted by your post I checked my cameras and did pick it up. The screengrab here shows it and the video at the link below shows it slowly moving downwards towards the northern horizon.
https://nickdjames.com/Spacecraft/20250524_propvent/propvent2_20250624_001530_ndj.mp4
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That is very sad news. I remember seeing Terry and one of his early cameras at an Exhibition Meeting in the early nineties. I bought an early SX and was astonished by its capabilities. Terry was always incredibly helpful.
My first light with the SX was on 1994 September 1. The image of M57 doesn’t look much now but it was a revelation then. The chip was 510×256 pixels, the pixels weren’t square and the field of view was tiny but the sensor was much more sensitive than film and there was no messing around with horrible chemicals afterwards.
Terry led the way in the UK and changed my (astronomical) life completely.
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This interesting paper has jus been posted on Archiv:
https://arxiv.org/pdf/2506.11217
The authors consider the potential effect of a lunar impact of 2024 YR4 on 2032 December 22. They conclude that it could temporarily increase the flux of mm sized meteoroids in near-Earth space by several orders of magnitude. This could be bad news for spacecraft in low-earth orbit but might give us a nice meteor shower.
The probability of a lunar impact is currently around 4% and the high end of their flux predictions require some relatively unlikely alignments to happen but it is definitely an interesting read.
The latest prediction from Marco Langbroek is that re-entry will occur around 06:30 UTC tomorrow, May 10, with an uncertainty of +/- 4.1 hr:
https://sattrackcam.blogspot.com/2025/04/kosmos-842-descent-craft-reentry.html
The latest TLE from space-trak (dated March 9.655) has perigee down to 127 km. The spacecraft has passes over the UK on May 10 as follows (times are UTC):
04:34 – Low elevation in the southeast.
06:05 – Almost overhead
07:36 – Almost overhead
09:06 – Low in the southwest.All of these are in daylight so if it does re-enter over the UK we are unlikely to see it but, if the sky is clear it might be worth looking when it comes over.
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Unfortunately we don’t have any night-time passes of this spacecraft coming up.
This page will get updated as the TLEs get updated:
https://aerospace.org/reentries/6073
The current re-entry prediction is 2025 May 10 04:42 UTC +/- 19 hours.
The conditions were slightly better low to my northwest this evening and the comet is more obvious in this stack:
https://nickdjames.com/Comets/2025/2025F2/2025f2_20250429_203939_ndj.jpg
My image of this nebula at 0.56 arcsec/pix taken this morning (April 29.06) shows quite a bit of detail in the brighter part of the nebula. Certainly an interesting object to follow.
https://britastro.org/observations/userimg/20250429_202133_f7c854744716.jpg
I got a possible detection of the remnants of this comet last night (April 28.86) from Chelmsford, low in the bright evening twilight.
https://britastro.org/observations/observation.php?id=20250429_063941_2990db2ceeed4e3a
Yes, the ion tail is straightforward since it consists of ions accelerated away from the coma entrained in the solar wind and so it extends radially along the anti-Sun vector. That is easy to calculate.
The dust tail is an orbital mechanics problem. Each dust grain leaves the nucleus at a particular velocity and then it gets accelerated, mainly by solar radiation pressure. The acceleration depends on the mass of the grain and its cross sectional area. Because of this acceleration, each grain moves in a slightly different orbit to the nucleus but the difference in velocities is relatively small and so the grains spread out from the nucleus in the comet’s orbital plane. There are some good online demonstrations of how this is modelled:
https://www.comet-toolbox.com/FP.html
https://hdr-astrophotography.com/comet-tails-simulations/One of the most spectacular dust tails of recent times was that of C/2006 P1 (McNaught):
https://britastro.org/cometobs/2006p1/thumbnails.html
A detailed description of how that was modelled is here:
https://www.sciencedirect.com/science/article/pii/S0019103518301192
