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Re: Comet of the century or pipe dream?

 

Mag 34 for JWST is ultra-deep field like when Hubble reaches mag 31+. I'm not convinced that they would make such an ultra-deep field just to recover such a comet that would anyway be recovered long before perihelion by more classical telescopes, unless one really has a good reason for such an observation, or has something else more certain to observe in this field.

Adrien


Le dim. 4 mai 2025, 16:12, Maik Meyer via <maik=[email protected]> a ¨¦crit?:
Thanks Rob!

> "Some people want to achieve immortality through their works or their descendants. I prefer to achieve immortality by
> not dying."
>
> So far, so good, therefore maybe I'll live long enough (and/or technology will improve fast enough) for me to witness
> the recovery of this comet while I'm a "young" centenarian (and not that long after the next return of 1P/Halley!) ? --Rob

All,

coming back to the possibility of recovery attempts in the coming decades. I really hope it would be possible withing
the next 20 years.

And I really wonder...

I've read somewhere that JWST is able to down to 34 mag! The Deep Field at least showed objects that faint. Integration
time must have been quite long. So, I assume it should be possible, technically, already now if one really knows where
to look.

Regards

Maik
--
"One cannot discover comets lying in bed." * Lewis Swift
________________________________________________________________________









Re: Comet of the century or pipe dream?

 

Thanks Rob!

"Some people want to achieve immortality through their works or their descendants. I prefer to achieve immortality by not dying."
So far, so good, therefore maybe I'll live long enough (and/or technology will improve fast enough) for me to witness the recovery of this comet while I'm a "young" centenarian (and not that long after the next return of 1P/Halley!) ? --Rob
All,

coming back to the possibility of recovery attempts in the coming decades. I really hope it would be possible withing the next 20 years.

And I really wonder...

I've read somewhere that JWST is able to down to 34 mag! The Deep Field at least showed objects that faint. Integration time must have been quite long. So, I assume it should be possible, technically, already now if one really knows where to look.

Regards

Maik
--
"One cannot discover comets lying in bed." * Lewis Swift
________________________________________________________________________


Re: Comet of the century or pipe dream?

 

¿ªÔÆÌåÓý

Hi Maik: very nicely done! To borrow from Woody Allen:

?

"Some people want to achieve immortality through their works or their descendants. I prefer to achieve immortality by not dying."

?

So far, so good, therefore maybe I'll live long enough (and/or technology will improve fast enough) for me to witness the recovery of this comet while I'm a "young" centenarian (and not that long after the next return of 1P/Halley!) ? --Rob


Remnants of Comet C/2025 F2 (SWAN)

 

On the evening of 2025 April 29 Comet C/2025 F2 (SWAN) had a 9' long tail at a position angle of 349 degrees from where the comet coma use to be before the comet disintegrated. On the evening of 2025 May 2 the tail was not evident beyond the disintegrated debris field in the 4.8' wide aperture diameter circle, at least not in the 50mm f/5 Refractor and IMX462 camera. Using the 4.8' wide aperture diameter circle to encompass the major part of the disintegrated comets debris field the comet remnants magnitude was 8.5 on April 29 and 8.6 on May 2. There were no stars brighter than magnitude 15 in either 4.8' wide aperture diameter circle and the faintest stars in all images was about magnitude 14. The images were taken at an altitude of 4 to 5 degrees just as twilight was fading and before the comet sank into the atmospheric haze.


Re: Possible detection of C/2025 F2 on April 28.86

 

Hi Thomas, Nick at all, my last image of the "Perihelium" of the Comet C/2025 F2 SWAN....
Very clear sky, despite moon light and light pollution...
68x7 sec at 1,84 Sec per Pixel with C14 F7,5 and CCD
Best Regards?
Andrea Aletti?
MPC 204


Il mer 30 apr 2025, 08:50 Thomas Lehmann via <t.lehmann=[email protected]> ha scritto:

Nick, Andrea,

thanks for your update on successful observations, great achievment! It is quite
a challenge to image this fuzzy dust cloud and all depends on athmospherical
conditions. Despite fairly good weather the last few days, there has been the
usual haze and cirrus around at my site, so I could not image the comet again.

Thomas



> Am Wed, 30 Apr 2025 08:33:02 +0200
> schrieb "Andrea Aletti via " <aletti.andrea=[email protected]>:
>
> Dear all, from Schiaparelli Observatory the ex comet C2025 F2 near the NW
> Horizon two days ago in excellent sky condition
> Best Regards
> Andrea Aletti e Federico Bellini MPC204
>
> Il giorno mar 29 apr 2025 alle ore 23:46 Nick James via <comets=
> [email protected]> ha scritto:?
>
> > Thomas,
> >
> > Thanks. That's a great image. I've be plagued by distant cirrus near the
> > horizon to my northwest (probably aircraft contrails) so my transparency
> > has not been very good. I did have slightly better conditions tonight
> > (April 29.86) and the comet is more obvious in this stack:
> >
> >
> >
> > Nick.
> >
> >
> > On 29/04/2025 11:28, Thomas Lehmann via wrote:?
> > > Two nights earlier I have had a chance to observe whats left of the?
> > comet from?
> > > Weimar, Germany. The comet was at an altitude of only 5.5¡ã above horizon?
> > but I?
> > > gave it a try with my RASA 11" and ASI6200MC as conditions were?
> > exceptionally?
> > > good for my location.
> > > The brightness near the head (green color channel) as measured within an
> > > aperture of 3' is
> > >? ? 2025 04 26.84 UT, m=9.8mag
> > > and the tail extent is about 20' at P.A.=333¡ã
> > >
> > > I am attaching the stacked image (12 minutes total exposure time) and an
> > > inverted star trail subtracted and stronger smoothed image to highlight?
> > the?
> > > dust tail.
> > >
> > > Out of curiosity I am attaching a plot of differential extinction?
> > measured from?
> > > stars near the comet as it is taken into account by my AIRTOOLS software
> > > automatically.
> > >
> > > CS
> > > Thomas
> > >
> > >?
> > >> Am Tue, 29 Apr 2025 07:42:48 +0100
> > >> schrieb "Nick James"<comets@...>:
> > >>
> > >> Possible detection of C/2025 F2 (SWAN) on April 28.86:
> > >>
> > >>?
> > ?
> > >>
> > >> A very noisy image taken in very bright twilight but there is a faint
> > >> patch of material at the right location.
> > >>
> > >> Nick James. BAA
> > >>
> > >>
> > >>
> > >>
> > >>
> > >>?
> >
> >
> >
> >
> >
> >
> >?
>
>
>
>
>






Re: C/2024 G3 ATLAS orbital plane crossing

 

¿ªÔÆÌåÓý

Just a follow up on this,

I tried a visual observation this morning using 15x70mm binoculars, but estimated fainter than mag 10.

Here¡¯s an image of C/2024 G3 ATLAS on 2025 April 30 at 19:30UT.

Using a Canon 6D + Sigma 200mm f/2.8. 12x30sec iso3200. FOV 8 deg. North left.

I estimate the total tail length at 6 degrees in PA12.

This comet is 2.67AU from Earth!

?

Cheers,

Michael

?

From: [email protected] <[email protected]> On Behalf Of Michael Mattiazzo via groups.io
Sent: Wednesday, 30 April 2025 8:42 PM
To: [email protected]
Subject: [comets-ml] C/2024 G3 ATLAS orbital plane crossing

?

Hi all

?

FYI.

Earth is now crossing the orbital plane of Ghost comet C/2024 G3 ATLAS.

This Image was taken on 2025 April 30 at 09:15UT using a remote telescope ITEL-T70 Chile 135 mm f/3.5 Samyang Lens + CMOS. 10x60sec. FOV 7 deg. North right.

The dust trail in this image, viewed edge-on, is at least 4 degrees long in PA13.

Star above centre is Psi Phe. Delta Phe is below left.

Total magnitude of the comet is difficult to ascertain, (approx mag 10) but visual attempts are encouraged.

Best situated for southern observers in the morning sky.

Despite its disintegration in January, it keeps on giving. ?

?

Cheers,

Michael


Re: C/2024 G3 ATLAS orbital plane crossing

 

Great image! Unforgettable Comet!?
Regard

Il mer 30 apr 2025, 12:42 Michael Mattiazzo via <mmatti=[email protected]> ha scritto:

Hi all

?

FYI.

Earth is now crossing the orbital plane of Ghost comet C/2024 G3 ATLAS.

This Image was taken on 2025 April 30 at 09:15UT using a remote telescope ITEL-T70 Chile 135 mm f/3.5 Samyang Lens + CMOS. 10x60sec. FOV 7 deg. North right.

The dust trail in this image, viewed edge-on, is at least 4 degrees long in PA13.

Star above centre is Psi Phe. Delta Phe is below left.

Total magnitude of the comet is difficult to ascertain, (approx mag 10) but visual attempts are encouraged.

Best situated for southern observers in the morning sky.

Despite its disintegration in January, it keeps on giving. ?

?

Cheers,

Michael

?


Re: C/2024 G3 ATLAS orbital plane crossing

 

Wow, very nice images Michael and Rob of the 3+ month disintegrated comet.?

Cheers, Erik


Re: C/2024 G3 ATLAS orbital plane crossing

 

Nice work Michael! here's my shot from tonight, with 6.4 degrees of tail visible. What a change from a few weeks ago.
?
Cheers -
?
Rob Kaufman
?


C/2024 G3 ATLAS orbital plane crossing

 

¿ªÔÆÌåÓý

Hi all

?

FYI.

Earth is now crossing the orbital plane of Ghost comet C/2024 G3 ATLAS.

This Image was taken on 2025 April 30 at 09:15UT using a remote telescope ITEL-T70 Chile 135 mm f/3.5 Samyang Lens + CMOS. 10x60sec. FOV 7 deg. North right.

The dust trail in this image, viewed edge-on, is at least 4 degrees long in PA13.

Star above centre is Psi Phe. Delta Phe is below left.

Total magnitude of the comet is difficult to ascertain, (approx mag 10) but visual attempts are encouraged.

Best situated for southern observers in the morning sky.

Despite its disintegration in January, it keeps on giving. ?

?

Cheers,

Michael

?


Comet C/2025 F2 (SWAN) > 2025.04.29 from BBO

 

Hello,

a recent photo of the remnants of comet C/2025 F2 (SWAN) taken by BBO
on 2025.04.29



Best,
BBO


Re: Possible detection of C/2025 F2 on April 28.86

 

Nick,
??????? thanks for the photo. I now realise that I also caught the patchy remnants of the comet about 20-30 minutes after your picture. Photo was taken April 29.91 with a Seestar 50 for 4 minutes and then cropped. There are some power lines towards the top of the photo.

Kind regards

Stephen McCann
Southampton, UK (N 50¡ã 56.50', W 001¡ã 27.90')
F2SWAN-stephen-mccann.jpg


On Wed, 30 Apr 2025 at 07:33, Andrea Aletti via <aletti.andrea=[email protected]> wrote:
Dear all, from Schiaparelli Observatory the ex comet C2025 F2 near the NW Horizon two days ago in excellent sky condition
Best Regards
Andrea Aletti e Federico Bellini MPC204

Il giorno mar 29 apr 2025 alle ore 23:46 Nick James via <comets=[email protected]> ha scritto:
Thomas,

Thanks. That's a great image. I've be plagued by distant cirrus near the
horizon to my northwest (probably aircraft contrails) so my transparency
has not been very good. I did have slightly better conditions tonight
(April 29.86) and the comet is more obvious in this stack:



Nick.


On 29/04/2025 11:28, Thomas Lehmann via wrote:
> Two nights earlier I have had a chance to observe whats left of the comet from
> Weimar, Germany. The comet was at an altitude of only 5.5¡ã above horizon but I
> gave it a try with my RASA 11" and ASI6200MC as conditions were exceptionally
> good for my location.
> The brightness near the head (green color channel) as measured within an
> aperture of 3' is
>? ? 2025 04 26.84 UT, m=9.8mag
> and the tail extent is about 20' at P.A.=333¡ã
>
> I am attaching the stacked image (12 minutes total exposure time) and an
> inverted star trail subtracted and stronger smoothed image to highlight the
> dust tail.
>
> Out of curiosity I am attaching a plot of differential extinction measured from
> stars near the comet as it is taken into account by my AIRTOOLS software
> automatically.
>
> CS
> Thomas
>
>
>> Am Tue, 29 Apr 2025 07:42:48 +0100
>> schrieb "Nick James"<comets@...>:
>>
>> Possible detection of C/2025 F2 (SWAN) on April 28.86:
>>
>>
>>
>> A very noisy image taken in very bright twilight but there is a faint
>> patch of material at the right location.
>>
>> Nick James. BAA
>>
>>
>>
>>
>>
>>







Re: Possible detection of C/2025 F2 on April 28.86

 

Nick, Andrea,

thanks for your update on successful observations, great achievment! It is quite
a challenge to image this fuzzy dust cloud and all depends on athmospherical
conditions. Despite fairly good weather the last few days, there has been the
usual haze and cirrus around at my site, so I could not image the comet again.

Thomas

Am Wed, 30 Apr 2025 08:33:02 +0200
schrieb "Andrea Aletti via groups.io" <aletti.andrea@...>:

Dear all, from Schiaparelli Observatory the ex comet C2025 F2 near the NW
Horizon two days ago in excellent sky condition
Best Regards
Andrea Aletti e Federico Bellini MPC204

Il giorno mar 29 apr 2025 alle ore 23:46 Nick James via groups.io <comets=
[email protected]> ha scritto:

Thomas,

Thanks. That's a great image. I've be plagued by distant cirrus near the
horizon to my northwest (probably aircraft contrails) so my transparency
has not been very good. I did have slightly better conditions tonight
(April 29.86) and the comet is more obvious in this stack:



Nick.


On 29/04/2025 11:28, Thomas Lehmann via groups.io wrote:
Two nights earlier I have had a chance to observe whats left of the
comet from
Weimar, Germany. The comet was at an altitude of only 5.5¡ã above horizon
but I
gave it a try with my RASA 11" and ASI6200MC as conditions were
exceptionally
good for my location.
The brightness near the head (green color channel) as measured within an
aperture of 3' is
2025 04 26.84 UT, m=9.8mag
and the tail extent is about 20' at P.A.=333¡ã

I am attaching the stacked image (12 minutes total exposure time) and an
inverted star trail subtracted and stronger smoothed image to highlight
the
dust tail.

Out of curiosity I am attaching a plot of differential extinction
measured from
stars near the comet as it is taken into account by my AIRTOOLS software
automatically.

CS
Thomas


Am Tue, 29 Apr 2025 07:42:48 +0100
schrieb "Nick James"<comets@...>:

Possible detection of C/2025 F2 (SWAN) on April 28.86:



A very noisy image taken in very bright twilight but there is a faint
patch of material at the right location.

Nick James. BAA














Re: Possible detection of C/2025 F2 on April 28.86

 

Dear all, from Schiaparelli Observatory the ex comet C2025 F2 near the NW Horizon two days ago in excellent sky condition
Best Regards
Andrea Aletti e Federico Bellini MPC204


Il giorno mar 29 apr 2025 alle ore 23:46 Nick James via <comets=[email protected]> ha scritto:
Thomas,

Thanks. That's a great image. I've be plagued by distant cirrus near the
horizon to my northwest (probably aircraft contrails) so my transparency
has not been very good. I did have slightly better conditions tonight
(April 29.86) and the comet is more obvious in this stack:



Nick.


On 29/04/2025 11:28, Thomas Lehmann via wrote:
> Two nights earlier I have had a chance to observe whats left of the comet from
> Weimar, Germany. The comet was at an altitude of only 5.5¡ã above horizon but I
> gave it a try with my RASA 11" and ASI6200MC as conditions were exceptionally
> good for my location.
> The brightness near the head (green color channel) as measured within an
> aperture of 3' is
>? ? 2025 04 26.84 UT, m=9.8mag
> and the tail extent is about 20' at P.A.=333¡ã
>
> I am attaching the stacked image (12 minutes total exposure time) and an
> inverted star trail subtracted and stronger smoothed image to highlight the
> dust tail.
>
> Out of curiosity I am attaching a plot of differential extinction measured from
> stars near the comet as it is taken into account by my AIRTOOLS software
> automatically.
>
> CS
> Thomas
>
>
>> Am Tue, 29 Apr 2025 07:42:48 +0100
>> schrieb "Nick James"<comets@...>:
>>
>> Possible detection of C/2025 F2 (SWAN) on April 28.86:
>>
>>
>>
>> A very noisy image taken in very bright twilight but there is a faint
>> patch of material at the right location.
>>
>> Nick James. BAA
>>
>>
>>
>>
>>
>>







Re: Possible detection of C/2025 F2 on April 28.86

 

Thomas,

Thanks. That's a great image. I've be plagued by distant cirrus near the horizon to my northwest (probably aircraft contrails) so my transparency has not been very good. I did have slightly better conditions tonight (April 29.86) and the comet is more obvious in this stack:



Nick.

On 29/04/2025 11:28, Thomas Lehmann via groups.io wrote:
Two nights earlier I have had a chance to observe whats left of the comet from
Weimar, Germany. The comet was at an altitude of only 5.5¡ã above horizon but I
gave it a try with my RASA 11" and ASI6200MC as conditions were exceptionally
good for my location.
The brightness near the head (green color channel) as measured within an
aperture of 3' is
2025 04 26.84 UT, m=9.8mag
and the tail extent is about 20' at P.A.=333¡ã
I am attaching the stacked image (12 minutes total exposure time) and an
inverted star trail subtracted and stronger smoothed image to highlight the
dust tail.
Out of curiosity I am attaching a plot of differential extinction measured from
stars near the comet as it is taken into account by my AIRTOOLS software
automatically.
CS
Thomas

Am Tue, 29 Apr 2025 07:42:48 +0100
schrieb "Nick James"<comets@...>:

Possible detection of C/2025 F2 (SWAN) on April 28.86:



A very noisy image taken in very bright twilight but there is a faint
patch of material at the right location.

Nick James. BAA






Re: Comet of the century or pipe dream?

 

Hello Nico,

thanks for your comments and your simulations.

Regarding the discrepancies I think all depends on the setting of parameters which of course inhibit certain uncertainties. You'll see that the simulations I did from a simple selection of parameters with another tool showed a good agreement with the observations of 1402. Are they definite? Certainly not, but they show it is possible. I also do not really think that the perihelion date for 1402 can be so far off from March 25 as stated in the final paragraph in the respective chapter.

Concerning the descriptions which apparently do not seem to fit one also has to keep in mind that we deal with century-old or even millenia-old records which may have been altered, incorrectly recorded and transferred, or simply translated or interpreted wrongly. This is also outlined in the paper, where records are presented which contradict each other diametrically. We simply cannot take everything literally.

Also, we have to keep in mind that comets may behave not consistently, but this we all know. :-)

And, last but not least, and this should clearly be stated - this is a theory. We will probably not know until the end of this century if it is correct. I am positive, but who am I? :-)

Regards

Maik
--
"One cannot discover comets lying in bed." * Lewis Swift
________________________________________________________________________


Re: Comet of the century or pipe dream?

 

Hi Maik and Gary,

That is a fascinating paper,?congratulation for the?huge work behind this !
I could not resist running simulations of the tails of the comet for the different passages mentioned in your paper. I point out that there is no individual adjustment of the comets (besides orbital parameters, brightness parameters and dust/gas ratio) on my simulations. For instance, all the comets generate periodic modulation of dust production rate but the associated striations only show up if the geometry and perihelion distance allows it.?
The gif files can be opened with software like to be able to pause and extract single simulations.

1744:?
already simulated on my website, very good match between simulation and observation

1402:?
the simulation matches very well the observations, no comparison with the Hind orbit of the comet for which the simulation was no match at all. The only notable difference between simulation and reports I see is that, with perihelion date on March 25th calculated, the striation/multiple tails would probably only show up in the morning between 31st of March and 3rd of April, while they were reported on 26th and 27th of March. Does it seem possible that the perihelion date occurred a few days earlier ??

1032:?
the mention that the comet of 1032 had a rayed tail does not seem to match, as with the proposed orbit the comet would have been observed well before the perihelion passage, hence way before any significant striation could have developed. Thus, I am a bit perplexed by this.

676:
the simulation shows that the comet would have been rather ¡°small¡± in August and September and become ¡°great¡± only around October. The ¡°turning back of the tail¡± does not seem to match neither striation, nor curved tail, nor a shortening of the tail mentioned in the paper as the tail should have kept lengthening over the whole apparition. I am also a bit perplexed by the descriptions on this one too.

2097:?
despite the excellent visibility, the fact that the earth will be near the orbital plane of the comet and the comet observed pre-perihelion, the comet should show much less interesting structure than in 1744. So probably another comet could be the actual comet of the century, I keep my fingers crossed that it would show up in a reasonable timespan!

Nicolas Lefaudeux


Le?mar. 29 avr. 2025 ¨¤?00:13, Qicheng Zhang via <qzalaska=[email protected]> a ¨¦crit?:
A fragment separating from the nucleus at a typical ~1 m/s at perihelion would have a difference in orbital period of +/-6 years. Being an instrinsically bright comet with a presumably large nucleus likely tens of kilometers in size, fragment separation might be a bit faster, perhaps up to 10x that. In this case, some fragments from the last apparition, if any, could start appearing fairly soon.

Qicheng

On Monday, April 28, 2025 at 02:51:07 p.m. MST, Adrien Coffinet via <adrien.coffinet2=[email protected]> wrote:


After reading a comment on Facebook, I'm wondering how likely it is that there could exist smaller fragments of this comet, that would have been unobservable in the 18th century or before, but that would be observable now or later in the century.

And if so, assuming a typical separation speed, what could we expect as the order of magnitude of delay between the perihelion of such a fragment and that of the main fragment, assuming that it separated N perihelia ago? (At first order, and unless there is a close approach with some planet, I'm assuming that it should be some typical interval corresponding to a separation one perihelion ago, multiplied by N.)

Adrien


Le lun. 28 avr. 2025, 18:00, Maik Meyer via <maik=[email protected]> a ¨¦crit?:
Qicheng,

> Very interesting! Do you know what the uncertainty on its angular elements looks like? For multi-apparition objects
> observed only near perihelion, the positional uncertainty is generally dominated by those rather than the timing.

This is the 2097 orbit, "linked" to 1402 with a fixed perihelion date for 1402 which gave the best agreement with the
other apparitions.

Orbital elements:? C/1743 X1
? ? Perihelion 2097 Dec 8.61308 TT;? Constraint: Tp=1402 03 25.16
Epoch 2097 Dec 13.0 TT = JDT 2487320.5? ?Earth MOID: 0.3401? ?Ju: 0.1937
M? ?0.01103081? ? ? ? ? ? ? ? ? ? ? Sa: 0.9243? ? ? ? ? ? ? ? ? ?Meyer
n? ?0.00251447? ? ?Peri.? 151.44926
a? 53.5596075? ? ? Node? ? 49.79851
e? ?0.9957914? ? ? Incl.? ?46.66218? ? ? ? ? ? ? ? ? ? ? ?(J2000 ecliptic)
P 391.97293? ? ? ? ? q 0.22541007? Q 106.893805
110 of 120 observations 1743 Dec. 15-1744 Mar. 4; mean residual 31".95

Here are the sigmas for the angular elements.

sigma_i? ? ? ? ?0.046 deg
sigma_omega? ? ?0.031 deg
sigma_node? ? ? 0.08 deg

> There's a chance it could be already be observable right now if you know exactly where it is. If its nucleus is
> comparable in brightness to that of Hale-Bopp's (H=9), it would be mag ~29 now at r=96 au. If it has the same normalized
> level of dust activity as Hale-Bopp (i.e., 2 mag fainter) and a more typical nucleus albedo (i.e., ~4%), it would be ~3
> mag fainter at mag ~32. Toward the brighter end, it might be a reasonable target for the Roman Space Telescope to
> recover (if that telescope isn't cancelled...).

I wonder what else you'll find if you go down to 30 mag....

:-)

Maik
--
"One cannot discover comets lying in bed." * Lewis Swift
________________________________________________________________________









Re: Possible detection of C/2025 F2 on April 28.86

 

Two nights earlier I have had a chance to observe whats left of the comet from
Weimar, Germany. The comet was at an altitude of only 5.5¡ã above horizon but I
gave it a try with my RASA 11" and ASI6200MC as conditions were exceptionally
good for my location.
The brightness near the head (green color channel) as measured within an
aperture of 3' is
2025 04 26.84 UT, m=9.8mag
and the tail extent is about 20' at P.A.=333¡ã

I am attaching the stacked image (12 minutes total exposure time) and an
inverted star trail subtracted and stronger smoothed image to highlight the
dust tail.

Out of curiosity I am attaching a plot of differential extinction measured from
stars near the comet as it is taken into account by my AIRTOOLS software
automatically.

CS
Thomas

Am Tue, 29 Apr 2025 07:42:48 +0100
schrieb "Nick James" <comets@...>:

Possible detection of C/2025 F2 (SWAN) on April 28.86:



A very noisy image taken in very bright twilight but there is a faint
patch of material at the right location.

Nick James. BAA






Possible detection of C/2025 F2 on April 28.86

 

Possible detection of C/2025 F2 (SWAN) on April 28.86:



A very noisy image taken in very bright twilight but there is a faint patch of material at the right location.

Nick James. BAA


Re: Comet of the century or pipe dream?

 

A fragment separating from the nucleus at a typical ~1 m/s at perihelion would have a difference in orbital period of +/-6 years. Being an instrinsically bright comet with a presumably large nucleus likely tens of kilometers in size, fragment separation might be a bit faster, perhaps up to 10x that. In this case, some fragments from the last apparition, if any, could start appearing fairly soon.

Qicheng

On Monday, April 28, 2025 at 02:51:07 p.m. MST, Adrien Coffinet via groups.io <adrien.coffinet2@...> wrote:


After reading a comment on Facebook, I'm wondering how likely it is that there could exist smaller fragments of this comet, that would have been unobservable in the 18th century or before, but that would be observable now or later in the century.

And if so, assuming a typical separation speed, what could we expect as the order of magnitude of delay between the perihelion of such a fragment and that of the main fragment, assuming that it separated N perihelia ago? (At first order, and unless there is a close approach with some planet, I'm assuming that it should be some typical interval corresponding to a separation one perihelion ago, multiplied by N.)

Adrien


Le lun. 28 avr. 2025, 18:00, Maik Meyer via <maik=[email protected]> a ¨¦crit?:
Qicheng,

> Very interesting! Do you know what the uncertainty on its angular elements looks like? For multi-apparition objects
> observed only near perihelion, the positional uncertainty is generally dominated by those rather than the timing.

This is the 2097 orbit, "linked" to 1402 with a fixed perihelion date for 1402 which gave the best agreement with the
other apparitions.

Orbital elements:? C/1743 X1
? ? Perihelion 2097 Dec 8.61308 TT;? Constraint: Tp=1402 03 25.16
Epoch 2097 Dec 13.0 TT = JDT 2487320.5? ?Earth MOID: 0.3401? ?Ju: 0.1937
M? ?0.01103081? ? ? ? ? ? ? ? ? ? ? Sa: 0.9243? ? ? ? ? ? ? ? ? ?Meyer
n? ?0.00251447? ? ?Peri.? 151.44926
a? 53.5596075? ? ? Node? ? 49.79851
e? ?0.9957914? ? ? Incl.? ?46.66218? ? ? ? ? ? ? ? ? ? ? ?(J2000 ecliptic)
P 391.97293? ? ? ? ? q 0.22541007? Q 106.893805
110 of 120 observations 1743 Dec. 15-1744 Mar. 4; mean residual 31".95

Here are the sigmas for the angular elements.

sigma_i? ? ? ? ?0.046 deg
sigma_omega? ? ?0.031 deg
sigma_node? ? ? 0.08 deg

> There's a chance it could be already be observable right now if you know exactly where it is. If its nucleus is
> comparable in brightness to that of Hale-Bopp's (H=9), it would be mag ~29 now at r=96 au. If it has the same normalized
> level of dust activity as Hale-Bopp (i.e., 2 mag fainter) and a more typical nucleus albedo (i.e., ~4%), it would be ~3
> mag fainter at mag ~32. Toward the brighter end, it might be a reasonable target for the Roman Space Telescope to
> recover (if that telescope isn't cancelled...).

I wonder what else you'll find if you go down to 30 mag....

:-)

Maik
--
"One cannot discover comets lying in bed." * Lewis Swift
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