Welcome to Astrosite Groningen. On these pages you mainly find information, and a presentation of results, on a number of astronomical subjects that we find most interesting. Our main interests are comets and variable stars; therefore, emphasis will be on the various aspects of observing these objects (charts, observations, photographs). But we also plan to cover other topics, albeit only as an aside, such as eclipses, and atmospheric phenomena like aurora and noctilucent clouds, mainly by presenting a selection of our photographic results. We hope you enjoy this site. We always welcome comments, and suggestions for improvement. And feel free to contribute: observations, images, whatever you want to share... ![]() ![]() |
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Recent updates (over the last month) June 1, New APASS file for June. May 24, Observations of C/2019 L3, C/2019 T4, C/2019 U5, C/2020 K1, P/2023 E1 and 77P. May 4, Observation of C/2020 K1. New APASS file for May/June.
SQM-L sky brightness measurements at our observing sites. Click here.
NEW! June 1, a new file with comparison stars from APASS in the magnitude 10-15 range is available for the June moonless period.
Visually observable comets Comet Mv Trend Charts covered by APASS file C/2017 K2 (PANSTARRS) 11 fading no yes C/2019 L3 (ATLAS) 13 fading no yes C/2019 T4 (ATLAS) 13-14 fading no yes C/2019 U5 (PANSTARRS) 13-14 fading no yes C/2020 K1 (PANSTARRS) 12-13 near maximum no yes C/2020 V2 (ZTF) 10 near maximum no yes C/2021 S3 (PANSTARRS) 14 brightening no yes C/2021 T4 (Lemmon) 11 brightening no yes C/2021 X1 (Maury-Attard) 14-15 near maximum no yes C/2021 Y1 (ATLAS) 14-15 fading no yes C/2022 A2 (PANSTARRS) 11-12 fading no yes C/2022 E3 (ZTF) 12-13 fading no yes C/2022 L2 (ATLAS) 14-15 brightening no yes P/2023 E1 (ATLAS) 10-11 brightening no yes 29P/Schwassmann-Wachmann 1 - small elongation,regular outbursts no no 71P/Clark 14 near maximum no yes 77P/Longmore 14 fading no yes 126P/IRAS 15 brightening no yes 185P/Petriew 12-13 brightening no yes 237P/LINEAR 12-13 near maximum no yes
Comet C/2021 A1 (Leonard) at perihelion
This comet, discovered a year ago as the first one of 2021 is passing perihelion today. Over the last couple of weeks it has developed into a very fine object in the evening sky, in particular for observers in the southern hemisphere. It is very active, producing modest brightness outburst every 4 days or so since the middle of december, and showing a spectacular tail in wide field images, unusual for a comet that never became brighter than about magnitude 3-4 in a dark sky. A good example is the image above which was taken less than 24 hours from perihelion by Michael Mattiazzo from SWAN Hill, NSW. Currently the comet is about magnitude 5 visually. It is expected to fade gradually over the coming weeks moving away from both the Earth and the Sun. [03-01-2022]
Bright comet C/2020 F3 (NEOWISE)!
This comet, discovered on March 27 by the NEOWISE satellite as a magnitude 17 object, brightened to 7th magnitude for southern hemisphere observers before disappearing in evening twilight en route to perihelion on July 3 at slightly under 0.30 AU from the Sun. In the meantime it had become evident that this was an 'old' object, and there was good hope that northern hemisphere observers would see a naked eye comet near about magnitude 3 deep in morning twilight shortly after perihelion. So it was a pleasant surprise that C/2020 F3 actually emerged as a first magnitude object sporting a bright dust tail that rapidly grew longer and longer over the last week as the comet could be seen higher above the horizon in a darker sky. The (binned) image to the right was obtained on the early morning of July 12 by Martin Mobberley from Cockfield, Suffolk, UK and is a fair representation
of what visual observers were able to see around the same time. Over the coming weeks comet NEOWISE, now placed in the evening sky, will fade fairly rapidly after its closest approach to the Earth - the minimum distance was 0.692 AU around 23.0 July - moving south and becoming better placed for more southerly observers. |
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