Dr Paul Leyland

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  • in reply to: Logging in to the new website #610135
    Dr Paul Leyland
    Participant

    The site logs me out after a period of inactivity. That is mildly annoying but nothing more.

    What is annoying is when I am logged out when the Forum page is displayed. To contribute I have to re-authenticate (fair enough) but after doing so I am not returned to the previously displayed page.

    Can this be fixed?

    in reply to: ASTAP #610078
    Dr Paul Leyland
    Participant

    I don’t (yet) use ASTAP but thanks for drawing it to my attention. I will take a look.

    Russ Laher’s Aperture Photometry Tool, APT, is my tool of choice. Written by a professional at the ZTF for professionals and amateurs alike it does a very good job very easily. It produces CSV format output which is easy to convert to a BAA-VSS spreadsheet. A script to do just that is available from me on request.

    APT is available from https://aperturephotometry.org/ and there’s a Wikipedia article at https://en.wikipedia.org/wiki/Aperture_Photometry_Tool

    A particularly nice feature of APT is that the apertures can be elliptical, so tracking errors can be tolerated better than with purely circular apertures.

    For plate solving I use a local installation of astrometry.net with the Gaia DR2 catalogue.

    in reply to: Mercury’s Sodium tail #610057
    Dr Paul Leyland
    Participant

    As Comet Section director I like planets that look like comets…

    I like comets that look like planets 😉

    Most of the small junk out in the solar system like Caliban, Nereid, Quaoar and Makemake would be brilliant comets if they came close enough to us.

    • This reply was modified 2 years, 3 months ago by Dr Paul Leyland. Reason: Fix [/quote] tag
    • This reply was modified 2 years, 3 months ago by Dr Paul Leyland.
    in reply to: Very slow possible nova in Vela #610052
    Dr Paul Leyland
    Participant

    Dec of -56 degrees is a bit far south even for La Palma. I will pass on this one.

    Dr Paul Leyland
    Participant

    On Twitter Martin Lewis asked about this event. The thread is available at https://twitter.com/SkyInspector/status/1520183595167481856

    https://twitter.com/richard_e_cole/status/1520217320819507205 suggests that it may have been a fuel dump from Cosmos 2555 as the orbit tallies rather closely.

    in reply to: Theta Aurigae – A Double Star? #609962
    Dr Paul Leyland
    Participant

    The nearest star, alpha Centauri, is 1.3 parsecs away and although it is a multiple system the separations are many AU and the orbital periods are much more than a decade.

    Thinking about it, if you are prepared to use a robotic telescope and/or travel to the southern hemisphere and are willing to relax your orbital period requirement to 80 years, alpha Cen is also a possibility.

    in reply to: Theta Aurigae – A Double Star? #609958
    Dr Paul Leyland
    Participant

    Thank you, that is very helpful. Now take a little time to think about some elementary geometry.

    The definition of a parsec is the distance at which one astronomical unit subtends one second of arc. A parsec is about 3.2 light years, and Jupiter orbits the sun at a distance of 5AU in 12 years. Seen from a parsec away, Jupiter would be at most 5″ from the sun. A more massive object would orbit more quickly at the same distance, or be further away for the same period, ’tis true, but we’re talking order of magnitude estimates here.

    The nearest star, alpha Centauri, is 1.3 parsecs away and although it is a multiple system the separations are many AU and the orbital periods are much more than a decade.

    The only one which stands a chance of meeting your requirement is Sirius which is 2.7 parsecs away and where the companion is at most 11″ from the primary; the orbital period is about 50 years. A fair number of people have imaged Sirius B, myself included (see the gallery), but it is far from being an easy object.

    Good luck!

    If you want to measure stellar movements over a short period of time I would suggest that you start with stars of high proper motion. Barnard’s star is the easiest target and its movement can be measured within a week or two if you are careful. It moves around 11″ per annum, or 1″ per month. Careful astrometry should be good to around 0.3″ with amateur equipment. Again, see the gallery for my animated GIF which shows the movement from one summer to the next.

    Paul

    • This reply was modified 2 years, 3 months ago by Dr Paul Leyland. Reason: Fix tyop
    • This reply was modified 2 years, 3 months ago by Dr Paul Leyland.
    in reply to: New website feedback #609929
    Dr Paul Leyland
    Participant

    Robin posted the above some hours ago. As is my usual habit I clicked on the “8 hours 43 minutes” link on the forum contents page which normally takes me to the last post in the thread so annotated.

    On this occasion it took me to the Reply-To: form, the one into which I am now typing. This behaviour was reproducible.

    My guess is that Robin’s post is the last one on the page and the javascript has a fence-post error which led it to create a new page.

    in reply to: Theta Aurigae – A Double Star? #609912
    Dr Paul Leyland
    Participant

    What do you regard as a “short period”?
    What do you regard as “wide”?

    Hard to give specific advice without answers to those questions.

    in reply to: Asteroidal whine #609686
    Dr Paul Leyland
    Participant

    Thanks Alan.

    At least in here in La Palma the temperature never falls below 5C, and that figure only exceptionally. I have experienced 7C on this visit, but that is unusual too and the lowest I have ever encountered. “Here” is Tacande at an altitude of 760m. Up on El Roque it falls well below zero every winter.

    I am also fortunate here in having a warm and lit control room, well-equipped with a kettle.

    Having spent many hours below freezing outside in the UK, with only a cat on occasion to keep my hands warm (another long story), I know well what you mean.

    in reply to: Ron Arbour #609685
    Dr Paul Leyland
    Participant
    in reply to: Moon solves Hubble tension #609563
    Dr Paul Leyland
    Participant

    Daryl wrote in https://britastro.org/forums/topic/moon-solves-hubble-tension#post-609557

    Do we have the embryo of a new BAA section the Jaffa Section as clearly there is a lot of research to be done especially with the variation of recipe’s around

    The Oxford University Astronomical Society conducted a great deal of research into the physics of the Jaffa Cake back in the 70’s and early 80’s. I can still remember some of the results and perhaps there are other ex-OUAS members of that era who are now BAA members.

    I seem to remember that the symmetry of the ground state ensemble was something like quintuplet-N-27/2 with at least four excited states known. The Jaffa Cake is not a fundamental particle in that it has substructure composed of chocons, jamons and cakons, the last of which decay into crumbons.

    It is a great pity that this topic came up too late for Heather Couper to contribute. I am certain that she partook in that research.

    in reply to: Ron Arbour #609535
    Dr Paul Leyland
    Participant

    i never met Ron, as far as I recall, but he did prompt me to submit my image of the globular clusters around M81 as a candidate for a picture of the week. The submission was successful. Thanks Ron!

    in reply to: Moon solves Hubble tension #609432
    Dr Paul Leyland
    Participant

    One of several such papers uploaded today.

    in reply to: New website feedback #609270
    Dr Paul Leyland
    Participant

    https://britastro.org/observations/observation.php?id=20181111_015500_44cd9ab1092010e3 contains a reference to https://britastro.org/node/19348 (this is just a specific example of no importance otherwise), which link is now broken. I can easily fix isolated examples in my own pages but perhaps they may be corrected globally with a script? AFAICT, and assuming the old pages are still available in an archive somewhere, a relatively straightforward pattern matching exercise should match old with new URLs.

    Priority: MAÑANA

    in reply to: Detection and observation of Earth impactor 2022 EB5 #609017
    Dr Paul Leyland
    Participant

    That lead to a fascinating, but rather bizarre, exchange on Twitter. It was noted that “giraffe” could be a unit of mass or of length. I proposed that the “slug” be used as that is a standard of unit of mass. Things got rather silly after that.

    in reply to: New website feedback #608597
    Dr Paul Leyland
    Participant

    https://britastro.org/forums/topic/new-website-feedback/page/3#post-608593

    Ah, I thought it must be (relatively easily) possible. Thanks.

    It doesn’t look like a link under Firefox (no underlining and no colour change, so I never thought of looking there. A combination of UBD and inadequate documentation perhaps.

    Paul

    P.S. If I can be assistance please ask.

    in reply to: New website feedback #608592
    Dr Paul Leyland
    Participant

    Second Robin’s post of 1:43 pm.

    It is a real PITA not to be able to link to posts to which I am replying.

    in reply to: New website feedback #608562
    Dr Paul Leyland
    Participant

    LazyFocus still doesn’t work despite everything I have tried. The contents of the RAR file are internally inconsistent. At least I now know where to ask for more help, so thanks again.

    in reply to: New website feedback #608556
    Dr Paul Leyland
    Participant

    Ah, the latest RAR file is markedly different from the one of several years ago. I am now rather more hopeful and will report back.

    Thanks again.

    Moderator: might this portion of the thread be better moved elsewhere, the equipment area perhaps?

Viewing 20 posts - 261 through 280 (of 713 total)