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STEREO data for the 19th and 20th:
https://nickdjames.com/STEREO/20230919.gif
https://nickdjames.com/STEREO/20230920.gifThe comet has been in the STEREO HI1 field of view since 17th Sept. The full res data is now available for the 17th and 18th.
Here’s an example for Sept 18:
http://nickdjames.com/STEREO/20230918.gif
Two nice tails.
Nick.
By coincidence I’m on La Palma at the moment. Last night I went up to the visitors’ centre which is around 2100m to look for the comet. Unfortunately there was a lot of cirrus out over the ocean in that direction but I did get a few images of the comet through thinner gaps. This one:
https://britastro.org/observations/observation.php?id=20230916_102938_2de129e1ecfdd06f
is a single 2s exposure with FoV 4×3 deg. The comet was 0.25 degrees above the theoretical horizon but refraction and my altitude made it appear more than a degree up.
It certainly wasn’t spectacular and it wasn’t visible in binoculars but it does show a bit of a tail if you zoom in.
I’m not expecting that C/2023 P1 will look anything like this but there have been reports of bright objects near the Sun in the past which may have been comets. A nice example is the object of 1921 seen from Mount Hamilton and possibly other places that is reported here:
https://adsabs.harvard.edu/full/1921JRASC..15..364P
Anyone who has been to Lick Observatory on Mount Hamilton can imagine that party looking out to the west towards the Pacific and seeing this mystery object appear briefly at sunset. We’ll probably never know what it was but they were experienced observers and a comet is a good bet.
This is a periodic comet which has been close to the Sun many times. Such comets tend to have a low dust/gas ratio which doesn’t bode well for a bright dust tail post-perihelion. It certainly has an impressive gas tail at the moment and it will be interesting to see how that develops over the next few weeks. Jaeger’s image shows it at 10 deg long so it might be visible in darker skies once the head has set.
Yes, you’re right, the media have hyped this comet up a lot and for most people it would be a real challenge since it is so close to the Sun in the sky. The elongation is now rapidly decreasing as it heads for perihelion so you will need very clear skies and a very low horizon and, preferably, a convenient mountain to see it over the next couple of weeks. It is an interesting object though and it does have a relatively short period (440 years) so I really should get a news item on the website. I’ll have a go at preparing something over the next few days.
This amazing image of it showing a 10 degree tail was taken from Austria this morning (Sept 7):
https://groups.io/g/comets-ml/message/31656
Michael Jaeger is one of the best comet imagers in the world and he has an excellent site.
Hi Duncan,
This comet is really close to the Sun in the sky so even if it does get bright it will be hard to find. It is currently very low in the morning sky in Leo but will soon move to very low in the evening sky as it approaches perihelion.
There was some discussion of it in the forum and on the comet section mailing list here:
https://britastro.org/forums/topic/a-good-year-for-japanese-astronomers
https://www.simplelists.com/baa-comet/msg/23154034/and there are plenty of images in our archive here:
Having a storm named after you is a great honour I guess and Skibbereen would be a good place to experience it!
I see that Met Éireann have also included Jocelyn after Jocelyn Bell Burnell, born in County Armagh, and the discoverer of pulsars (with some help from Tony Hewish).
I got another image of this comet this morning. It shows a faint ion tail to the west.
https://britastro.org/observations/observation.php?id=20230820_044052_9ecf5aeb201e50dfThe Japanese are very dedicated observers. The key strategy for amateur comet discovery is to scan the morning twilight since if a comet is in the right orbit it may appear here without being detected by the surveys. The attached plot shows the elongation of this comet, i.e. how far it appears to be from the Sun in the sky, as the purple line. The comet’s distance from the Sun and distance from the Earth are shown by the green and blue lines respectively. These lines are based on astrometry of the comet up to August 18 assuming that the orbit is a parabola, i.e. e=1.
You can see that the comet has been at an elongation of < 40 deg since the beginning of May and that Nishimura discovered it as it reached around 34 deg rising out of the morning twilight. As it approaches perihelion in September the elongation will drop rapidly and when the comet is at its brightest in September it will only be 12 deg or so from the Sun. To see it then you will probably want to be high up a mountain but we'll see. The surveys could have picked it up back in April when the elongation was much larger but it was then over 3au from the Sun and so would have been much fainter. I would expect that, once we have a better orbit, we'll find it somewhere in the survey data.
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I use a cheap barbecue cover bought from Amazon for my NEQ6 when it is left outside. It has survived some pretty torrential rainstorms this summer.
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I wonder what power level they used for their “interstellar shout”. DSS-43 has the capability to go to 400kW at S-band although I don’t think that has ever been used. Normal command uplinks are done at 70kW so they may have turned the wick all the way up for this. A 2-deg antenna offset is a loss of around 6dB so that would imply they would need nearly all of the 400kW to restore the link margin. Not much technical info on the NASA report though:
https://www.jpl.nasa.gov/news/nasa-mission-update-voyager-2-communications-pause
I’d put in the distance from memory. It is actually “only” 134au so that increases the angle a bit but not much. Sorry about that!
Yes, sending commands to Voyager 2 is a lot harder than receiving the telemetry. The spacecraft receiver is a bit unstable due to a capacitor failure and the noise temperature is high since the antenna is effectively looking at the Sun. The only ground station in the DSN that can command Voyager 2 is DSS-43 at Canberra. This has a huge 400kW power amplifier (the other 70-m stations have 20kW) but there are all sorts of restrictions on its use. I wouldn’t want to be a bird in the beam of that thing when it is transmitting at full power.
If you want some fun bedtime reading have a look at these links:
https://descanso.jpl.nasa.gov/DPSummary/Descanso4–Voyager_new.pdf
http://deepspace.jpl.nasa.gov/dsndocs/810-005/101/101E.pdf
https://deepspace.jpl.nasa.gov/dsndocs/810-005/relnotice49.pdf
https://space.stackexchange.com/questions/18956/has-dss-43-ever-been-used-in-high-power-mode-20-kw-for-an-emergency-situationThe spacecraft antenna pointing would be based on on-board sun and star tracker data so I assume they have a stored ephemeris for offsetting the pointing from the Sun to get peak gain towards the Earth. Voyager 2 is currently around 160au away so the Earth is always within 0.35 deg of the Sun anyway but this is what will happen in mid-October when it executes its next pointing update.
Voyager 2’s antenna is a 3.7-m diameter paraboloid and at S-band (2 GHz) a 2 degree pointing error would imply a link budget loss of around 6dB which is huge. It is probable that the 70-m DSN antenna at Canberra will be able to detect and lock to the residual downlink carrier but unlikely that they will be able to decode any data. They could decide to array lots of antennas to improve the downlink SNR but the main problem would be getting commands up to the spacecraft to reset the pointing.
Given the low science return from Voyager now it is probably easiest just to wait until the next antenna pointing update.
I got it at twilight this morning after a night of comet imaging. It was on its way out to apogee at a range of 120,000 km or so.
According to Horizons it should have been at 00 10 42.42 -04 00 27.0. The attached shows it a bit northeast of that but it looks as if the Horizons ephemeris is pretty good. This is a 60s exposure so the magnitude is meaningless since the image was trailed.
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Robin – That’s really impressive! Alan’s talk was really fascinating. I’m in awe of the precision of modern observational astronomy. I had no idea that we had directly detected comets around other stars through photometry or that we had seen variable absorption lines in high-resolution spectra which are inferred to be comets in the circumstellar disk of beta Pictoris. I need to do a lot more reading on this.
A fantastic day at the National Maritime Museum yesterday. We had over 100 people attend for a day of great talks about comets. My thanks to all the Flamsteed team and the people at the NMM who made the meeting possible, Dr. Greg Brown who gave us a great planetarium show, the speakers who were uniformly brilliant and to the audience who were really engaged and asked lots of excellent questions. My thanks also to Gill and Roger Perry who spent the day videoing the event. We’ll put the video online when it is ready.
If you did attend yesterday I hope you enjoyed the day and got home OK. I’m clearly biased since I think comets are the most interesting objects in the universe but with the direct observation of exocomets I think I can now extend my section’s reach to other star systems.
Thanks for that. ESA are tracking it and it is a shame that they haven’t publicly released any trajectory information. I’m not aware of any optical observations yet but it has been close to the Moon in the sky and it is at a far south declination. Once the Moon is out of the way I expect it will be picked up. I’ve been keeping an eye on NEOCP to see if any of the surveys get it.
ESA Ops did a small (2.1 m/s) trajectory correction the day after launch which implies that the Falcon 9 upper stage injection was very good. As far as I can tell everything is fine with the spacecraft.
