Geminids 2019 Backscatter Data

By Trevor Clifton

Pictured below is the backscatter data for the 24 hour period covering the Geminid maximum.

Some of the gaps in the data is due to high levels of RF interference which although the meteor data is logged in a text file its not printed on the graph as it may be unreliable.

Backscatter data covering the 24 hours of the Geminid maximum
Backscatter data covering the 24 hours of the Geminid maximum

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Lyrids Backscatter Data

By Trevor Clifton

The Lyrids may have been clouded out for visual observers, but Trevor managed to spot them using backscatter detection with his radio antenna.

The bar charts are produced in real time and a sample of the data log is attached.The first two bar charts show the run up to the event giving the background rate and the third the event itself.

Background detection rate in run up to the Lyrids (17th-18th April)
Background detection rate in run up to the Lyrids (17th-18th April)
Background detection rate in run up to the Lyrids (21st-22nd April)
Background detection rate in run up to the Lyrids (21st-22nd April)


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Comet 46P/Wirtanen

By Richard Harvey

46P/Wirtanen is a small short-period comet with a current orbital period of 5.4 years. It was discovered on January 17, 1948, by the American astronomer Carl Wirtanen, and expectations were high for the comet’s 2018 visit.

Many astronomers hoped for naked eye brightness reminiscent of 1997’s Hale Bopp, (which I remember seeing easily over the Albert Memorial from Queens Square, Wolverhampton. Hard to believe that was over twenty years ago!). Unfortunately, comet 46P/Wirtanen appeared fainter than hoped. At its closest approach, on the16th December 2018, it was only visible in binoculars from semi-rural sites. But even so, it gave amateur astronomers a fantastic, rare chance to study a comet.

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Trysull Observing Session 9th October 2018

By Richard Harvey

We held another observation session at our Trysull site on the 9th October. The sky was 100% clear from clouds for once, with a slight haze in the air as the evening drew on. Half a dozen members turned up at various times, and we were lucky to enjoy a very comfortable, mild, Autumn evening’s observing.

Three scopes were in use tonight. Steve bought along his Skywaytcher ED80 refractor with a go-to mount, and Martyn bought his pillar-mounted 110mm reflector. I took my Skywatcher 8” Reflector, so we were lucky once again in being able to use a range of different scopes.

Steve, aligning the go-to mount
Steve, aligning the go-to mount

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Trysull Observation Session Thursday 13th September 2018

By Richard Harvey

With Mars at its closest approach since 2003, and the prospect of a clear sky to view it, a last-minute observation session was hastily arranged for Thursday 13th September at our Trysull observation site. I took the society’s 12” dobsonian reflecting telescope (the Tom Collier Telescope), and several other members turned up, all hoping to get a fine display of planets.

The Moon was a waxing crescent in the west as we arrived, lit around 20%. Once the scope was set up, we all enjoyed fine views of the shimmering lunar landscape. I was particularly interested in the small craters in Mare Crisium, which were very noticeable. Crater Picard is 21 miles across, and Pierce is only 12 miles across, we could see them quite clearly. They will soon be washed out with sunlight and not viewable for another month. Quite distinct tonight, on the edge of Mare Crisium, was the distinct dramatic rises of Cape Cape Lavinium and Cape Olivium. 
To the left of the Moon, lower, just heading towards the trees, we saw Jupiter. With the sky not yet dark, the cloud belts were faint, but three of the moons were visible. The brightest, Ganymede, to the telescopic left. Although we could see only three moons, checking later with the Jovian Moon chart in Astronomy Now, all four should have been visible. Dimmer Callisto must have been lost to the twilight sky.

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Perseids Data

By Trevor Clifton

Given the sharp rise and fall the timings would suggest that the Earth travelled some 315,000 miles while in the debris stream from the comet.
It will be interesting to see if this figure changes next year.

Each bar in the chart is the meteor count for 10 minutes. 824 recorded for the 24 hours before and 1103 for the main day.

Meteor detection 24 hours before the expected peak
Meteor detection 24 hours before the expected peak
Meteor detection for the 24 hours during the peak of Perseid activity
Meteor detection for the 24 hours during the peak of Perseid activity


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M51 Mystery Object

By Trevor Clifton

During the evening of Saturday 14th April while commissioning a 150mm refractor some images were taken of M51. After processing the LRGB images and comparing the final image with stock internet images an object was spotted in our image which did not appear in those downloaded from the net.

Checking the subs, the mystery object only appeared in the first 120 second luminance image.

Searches to see if any asteroids were listed at these coordinates drew a blank. Clearly, the object is not a hot pixel so what is it? One explanation is that its a meteor trail which is head on to the field of view.

M51 with mystery object
M51 with mystery object
Close up crop of the M51 mystery object
Close up crop of the M51 mystery object

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