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David SwanParticipantC/2025 R2 via T59 at Siding Spring (1x60s; 2025/10/18 20:24). The apparent movement of the comet is quite fast at the moment: more than 11 arcsec/min.
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David Swan.
David SwanParticipantPleased to snap C/2025 R2 this evening, when it was low in the SW. Put the telescope on Phi Oph at about 7.15pm and waited for sky to darken.
12x10s, midpoint 2025/10/11 18:45 UT
MiniCat51 – Image Centre RA 16h 30m 48.5s, Dec -16° 40′ 04.6″ – Pos Angle +208° 40.5′- FL 173.6 mm, 8.94″/PixelAttachments:
David SwanParticipantI noticed this call in the Guardian too. And also thought it odd. Probably AI.
David SwanParticipantEph from MPC:
2025 04 08 0350 23 37 30.5 +26 11 37
My position
2025 04 08 0350 23 37 53.9 +26 14 53
David SwanParticipantCaptured this morning with my Seestar. Looking good!
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David SwanParticipantWill do. Was up this morning at 4am to observe, but there was a lot of cloud from the N to E. Of course it had all cleared by 9am…David
David SwanParticipantHaha. (Apart from this) I haven’t seen much April Fool’s Day content across the media. Serious times, I guess. David
David SwanParticipantAmazing.
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David SwanParticipantDevelopment of ion tail into at least three streamers.
MIDPOINT = ‘2023-01-29T20:59:22’ /UT of midpoint of exposureAttachments:
David SwanParticipantCaptured this eve (midpoint) 2023-01-28T19:12. Lovely ion tail.
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26 January 2023 at 2:38 pm in reply to: Asteroid 2023 BU: Space rock to pass closer than some satellites #615348
David SwanParticipantYes, that’s quite a rate of movement across the sky at Fri [corrected] 00:00 GMT. David
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This reply was modified 2 years, 9 months ago by
David Swan.
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David SwanParticipantSleeker ion tail when imaged last night. The comet’s hood lends it the appearance of a speeding bullet.
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David SwanParticipantMike and Martin,
Your posts prompted me to have look just now: they have indeed moved!!
You’re right Nick, there were / are some issues – I’ve seen a lot of hot pixels (not calibrating out), dead pixel columns and so on in my images. I’m less fastidious than you I suspect, so iTel is still more than good enough for me – for an astro fix when the weather is bad oop north. Let me know though if other remote observing solutions come your way – please.
David SwanParticipantFrom Discord forum:
mladen (iTelescope) — 10/01/2023 21:55
Our apologies. Overhauling all scopes after many years of service. Estimated at around 10 days work. Our team is in New Mexico Skies, working around the clock.mladen (iTelescope) — 12/01/2023 22:13
T02 (and all of New Mexico Skies) has been on extended maintenance from the 10th of January. This is scheduled to end by the 21st of January.
David SwanParticipantHello,
I observed on 29 days of 2022. By far my best month was December, followed by October then January. Comets were my main target, but I did also take pictures of assorted transients, globulars and other DSOs.
A poor year. But interestingly(?) I did observe on both the first and last days of 2022!
David
David SwanParticipantHi David. All looks good! Welcome.
David SwanParticipantNick,
I am not a member of the solar section, nor am I an expert on these matters. You may want to look here though:
https://hesperia.gsfc.nasa.gov/sftheory/questions.htm#AR_numbers
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I’ve seen reference to a formal naming system for sunspots. Where can this be found?
There is no naming or numbering system for sunspots. There is a system for numbering active regions, however. An active region can contain one or more spots. The National Oceanic and Atmospheric Administration (NOAA) numbers active regions consecutively as they are observed on the Sun. According to David Speich at NOAA, an active region must be observed by two observatories before it is given a number (a region may be numbered before its presence is confirmed by another observatory if a flare is observed to occur in it, however). The present numbering system started on January 5, 1972, and has been consecutive since then. An example of an active region “name” is “AR5128” (AR for Active Region) or “NOAA Region 5128”. Since we only see active regions when they are on the side of the Sun facing the Earth, and the Sun rotates approximately once every 27 days (the equator rotates faster than the poles), the same active region may be seen more than once (if it lasts long enough). In this case the region will be given a new number. Hence, a long-lived active region may get several numbers.
On June 14, 2002, active region number 10000 was reached. For practical, computational reasons, active region numbers continue to have only four digits. Therefore, the sequence of numbers is 9998, 9999, 0000, 0001, and so on. Active region number 10030, for example, is AR0030. This region will often simply be referred to as region number 30, with 10030 implied.
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David SwanParticipantPaul,
I think that PIPP, designed for lucky imaging crowd, can do animated gifs. The creator says it can be enjoyed with WINE.
https://sites.google.com/site/astropipp/
David
David SwanParticipantComet spectroscopy
JWST has been looking at the coma of C/2017 K2.
Will be interesting to see the results!
David SwanParticipantLikewise – negative for a PR Her outburst (8 May, 21:48 UT)
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