Saturday, 10 May 2025

May Flower Micro Moon

 May 12th sees the last of the year's Micro Moons. 

The opposite of a supermoon is a micromoon. That’s when the new or full moon reaches apogee or its greatest distance from Earth. A full micromoon appears about 12-14% smaller than a full supermoon and about 7% smaller than an average full moon.

 The Moon orbits the Earth in an ellipse, so there are times when it is closer to us and we see the Super Moon. At the other extreme, the Micro Moon appears smaller than normal, because it is farther away. If you miss this one, you will have to wait until next year.

The full moon in May is called the Flower Moon. The flowers in the fields and in the gardens are now becoming abundant for everyone to see.


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Friday, 9 May 2025

The Walter Goodacre Cooke telescope for sale in 1938

 In the journal of the British Astronomical Society from May 1938 there was an advertisement for a 10 inch Thomas Cooke offered by the executers of the late Walter Goodacre FRAS: together with an observatory with a 20-foot dome by Reid of Manchester. 

Price £500 or would sell telescope separately. There is also a sidereal clock by Home, Thornthwaite & Wood. 


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Thursday, 8 May 2025

Solar Eclipse seen from Ceylon in1871 with Cooke telescopes

 The solar eclipse on December 12th 1871 was most favourably observed at all the stations occupied by the scientific party under Mr Lockyer’s direction as well as by Mr Janssen. Important scientific results may be expected  to be shortly made known as indicated in the the message from Mr Lockyer.

 

Here in Colombo the weather during the eventful morning was all that could be desired, but being beyond the line of totality and shadow no special scientific value can be attached to the highly interesting observations made here by several gentlemen.

 

Our column this time will be unusually full of information respecting the eclipse and the special expeditions sent from home to observe it. About 3.5 inches of rain fell in Colombo between 8 00 pm on the 11th and 5.00 am on the 12th. We add the results of local observations:- the Sun rose obscured by clouds, which cleared off by about 6.30 .The whole surface of the Sun presented the usual strippled broken appearance, with here and there large spots. In the neighbourhood of these spots the strippling was more apparent than over the parts free of spots, but they came out in bold relief on the part of the Sun  close to the Moon’s limb. Probably this increase of distinctness was caused by contrast of the black spot &c of the dark limb of the moon. This could not be seen through the 3-inch telescope. Some little time before the greatest obscuration a halo was visible around the sun, which gave place to short bright rays. This latter appearance was probably an ocular deception, as no trace of it was visible through the 4.5-inch telescope under a low power.

 

At the greatest obscuration no trace of corona was observable through the same instrument, with a solar eyepiece with a power of about 30. This was carefully looked for. The unobscured portion of the sun, about 15-16ths of its disc, was well defined, without appendages of any kind. Towards the time of centrality the diminution of daylight was very conspicuous—going from the open air into the house it was very striking. Standing in the centre of the room, and looking through the open window, the sun-shine outside was of a neutral tint. The crows commenced to assemble on the tree-tops, cawing after their usual fashion, when preparing for their night's rest. The planet Venus, high in the sky, was distinctly visible to the naked eye, and Jupiter, low down in the western horizon, was plainly discernible with the aid of an opera-glass. The thermometer at the commencement of the eclipse indicated 91.5 °F  in the sun.  At 7-15 it showed a rise of 2.5 degrees and at the greatest phase it had  fallen to 84.5°.  In the shade it stood at 76 degrees; at 6-45 and at the greatest obscuration at 75°  At 9-10, with the full blaze of the then unobscured sun, the thermometer indicated 113 °; in the shade 81°.

 

 Mr. Van Dort, of the Surveyor- General's Department, with the aid of a 3-inch telescope, power 50, made some careful drawings of the different phases of the eclipse. The attempt to take the time of first contact and the ending of the eclipse proved abortive. An ordinary watch was the only time- keeper at hand.

 

Instruments used in the above observations : Equatorial Telescope by Cooke and Sons, of York, 4.5  inches clear aperture, 66 inches focal length. Telescope by same makers, 3 inches clear aperture, 42 inches focal length, mounted on tripod stand."

 

The above indicates the result of observations taken by Mr. Stainfurth Green at his residence in Colpetty. Mr. Stoddart, of the Surveyor- General's Office, took observations at the local observatory, showing the actual time to be

 

First contact 06 h 47m 30 s am 

Greatest darkness 07h.50 m15s

Last contact 09h.00 m 20s

 

Mr. W. L.H Skeen took some very successful photographic views, which show not only the progress of the eclipse, but the direction and form of the huge rays, projected from the sun or its corona, so much talked of.—Ceylon Observer.


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Wednesday, 7 May 2025

A little ramble through Caelum the Chisel

If I am being generous, I would say that the constellation of Caelum is rather faint, if I am being honest, it is one of the most obscure of all the 88 constellations. It is one of the 14 constellations created by the French astronomer Nicola Louis de Lacaille 1713-1762, it first appeared in his catalogue in 1763, and it is one of 14 constellations that he created while he was working in South Africa.

Originally called Caelum Sculptorium the Engravers’s Chisel, today it is referred to as just Caelum. It is a winter constellation that can be seen very low in the sky as seen from Britain below Orion the Hunter and to the east of the constellation of Lepus the Hare.

 It was apparently Francis Baily 1774-1844 who shortened the name of the constellation to the one we use today. Francis Baily is famous for his observations of the eclipse of the Sun in 1836 when he saw light beams coming through around the edge of the Moon through the canyons in between the mountains. He described them as bead of light and the term Bailys Beads has been used ever since.


I mentioned that is a dull constellation there are no bright stars. In fact, the brightest alpha is a magnitude 4.5 F class star meaning that it is hotter than the Sun and is 65 light years away. It is a double star, its companion of a faint red dwarf star. All the other stars in Caelum are fainter than alpha. This means that the slightest hint of mist or any light pollution or moonlight means it is impossible to find the constellation at all. An astronomy star map will show you where it is in the sky, but I doubt you will see any stars unless you use binoculars or telescopes to look for Caelum.

I can’t even say that there are any clusters of star or galaxies objects in Caelum worth looking at with telescopes because there really aren’t.

I have never been able to see any stars in this constellation even when observing from the south of England. I suppose if the sky was at its best and you knew exactly where you were looking you might just glimpse Caelum, but it is not worth the effort.

Even astronomers in the southern hemisphere would hardly give the area a second glance.


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Tuesday, 6 May 2025

Two transits of Mercury in 1878 and 1924 both seen with Cooke telescopes

Mercury is the closest planet to the Sun in our solar system and there will be times that it will pass in front of the Sun and can be seen as a small dot slowly moving across the face of the Sun. This is a Transit of Mercury, they occur on average 13 times per century, the last was in November 2019 the next will be in 2032. 

Here is a little-known astronomical fact, two transits of Mercury separated by 46 years which occurred on the same date and were both seen using Cooke of York telescopes. 

The transit of Mercury on May 7th 1878 (it was May 6th in the UK) was observed at 06 hours and 40 minutes as the Sun rose in Australia, with Mercury already halfway across the surface of the Sun, this observation was made by W J MacDonnell at Sydney using a 4.25 inch Cooke telescope.

 Then 46 years later in 1924 also on May 7th A F Bennett this time using a 6 inch Cooke telescope started observing a Transit of Mercury from 16 hours and 57 minutes from his home in Suffolk. 

Although he lived in Suffolk, he was actually born in Goole East Yorkshire and was educated at Bramham College.


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Monday, 5 May 2025

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE tonight and every Monday evening from 7.00 pm-9.00 pm on the award-winning Astronomy Show on Drystone Radio, probably the only regular astronomy show on any radio station in the country.

 I will take my weekly look at the night sky and look at all the latest news in astronomy. There will be the astronomical anniversaries this week plus the latest news from the astronomical societies in the north of England.


The Astronomy Show every Monday evening only on Drystone Radio live online at www.drystoneradio.com DAB radio in Bradford and East Lancashire, or 102 and 103.5 FM and can also be heard later on the Drystone Radio Podcast.

Cooke telescope on display at York Exhibition in 1881

 Yorkshire Gazette Saturday 7th May 1881

In the space intervening between the central and Great Halls, a large equatorial mounted telescope which stands 15 feet high is exhibited by Messrs T Cooke & Sons York opticians, the instrument which is an object of curiosity with an object glass of 10 inches. 

The sale price is £1200, today that telescope would cost over £186,000



                                                       www.theramblingastronomer.co.uk