Monday, 21 September 2026

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE 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.

 

A little ramble through Perseus

 Perseus was the hero of Greek mythology who rescued Andromeda who was chained to a rock waiting to be eaten by the Kraken Sea monster.

Andromeda’s mother Cassiopeia had upset Neptune god of the sea who then sent a monster the Kraken to attack her land. She was told the only way to save her land as to chain her daughter Andromeda to the Rocks and let the Kraken eat her.

Andromeda was chained to the rocks the monster appeared everything appeared lost but at the last-minute Perseus appeared riding the winged horse Pegasus. He had just killed the Medusa, a monster so horrible that anyone who looked at it would turn to stone. The medusa’ s hair was made of snakes. Perseus still had the head of the monster, he showed it to the Kraken which turned to stone. Perseus landed rescued Andromeda. They were married and lived happily ever after.

The Arab astronomers sometimes referred to Perseus as Hamil Ra’s al Ghul or the Bearer of the Demon’s Head.


The brightest star alpha has two given names Algenib which means Side or which can mean Elbow. It has a magnitude of 1.8 and is a F class supergiant with a surface temperature of 6,300 degrees and is 510 light years away.

Beta marks the eye of the medusa and its name is Algol which means the Winking Demon. It’s not one star but two which are eclipsing each other. This causes the brightness of the star to change. Astronomers call stars that change in brightness Variable Stars. This variability can be caused by several factors. The name Algol is interesting because the name might suggest that Arab astronomers 1,000 year ago knew it changed in brightness or winked in the sky. Sadly, we have no proof for this idea, yet.

This change in brightness of Algol was noted by the Italian astronomer Montanari in 1669. It would however not be until 1782 that the cause of the variability of Algol would be explained. It was the deaf astronomer John Goodricke who lived in York and  who explained what was happening to Algol.

Although he was deaf there was nothing wrong with his brain, he was very clever. He worked with another astronomer in York, Edward Pigott between 171-1786 when Goodricke died, they discovered and suggested what was causing light variations in some stars. They were literally hundreds of years ahead of their time with some of their thinking and ideas. When I was Curator of Astronomy at the Yorkshire Museum in York, I christened these two as the Fathers of Variable Star Astronomy.

John Goodricke suggested that the two stars were eclipsing each other in a regular period causing the light variations. He was right and his ideas of objects eclipsing stars and causing changes of light in stars is still used today as astronomers use the same theory and principals to find planets orbiting other stars.

The eclipse occurs every 2.8 days and the magnitude varies between 2.2 – 3.5. Algol lies at a distance of 90 light years and has a surface temperature of 13,000’C and is a B class star. The star which is eclipsing Algol cannot be seen with the eye.

Zeta has a magnitude of 2.9 and is a B class supergiant with a temperature of 20,500’C and is 750 light years away. There does not appear to be a name for this star.

Epsilon also has a magnitude of 2.9 and like zeta does not appear to have a name. Epsilon is also a B class star, with a temperature of 26,000’C and is 640 light years away.

NGC 869 and NGC 884 both with a magnitude of 3.7 and 3.8 respectively form the famous double cluster. They mark the sword of Perseus These are open clusters with 350 and 300 stars respectively, lying about 7,600 light years away and about 300 light years apart.  They are both visible to the naked eye but seen through binoculars they are spectacular.  Each cluster contains over 300 blue, white super giant stars. They are about 7,500 light years away.

One of the most spectacular meteor showers of the year is the Perseids which can be seen around the 12th/13th of August each year. Usually around 80 meteors per hour can be seen. The meteors or shooting stars as some people call them are small grains of dust left behind by a comet as it travels around the Sun.  There are several important meteor showers throughout the year. The comet connected with the Perseid meteor shower is comet Swift – Tuttle. 

While it was curious that Messier overlooked the double cluster maybe it was too obviously not a comet, he did however discover another open cluster in Perseus, this is M34 glimmering at mag 5.5 just visible to the naked eye to the right of Algol.


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Sunday, 20 September 2026

A little ramble through 19th century astronomy - Vulcan in 1876

 Nature November 16th 1876

Search for Intra Mercurial Planet

American observatories have been very diligent in the search for the supposed inter mercurial planet, no less than nine having given their whole time to the search on October 2,3,10 and 11 viz, those of Dartmouth college, Harvard College, Cincinnati, Glasgow (Mo), Washington, Albany, the Coast Survey in San Francisco, Ann Arbor, and the Observatory of Dr Peters, besides others that have made no report.

It is exceedingly creditable to the United States that they contain so many observatories, many of them of national ones, in which astronomical observations are so diligently pursued. 


                                                      www.theramblingastronomer.co.uk

Saturday, 19 September 2026

A little ramble through the Astronomical register January 1863 - The Elchies Equatorial

In the number of the ‘Monthly Notices’ for November last, will be found a very interesting account of the great equatorial telescope by the late Mr A Ross, which was shown at the 1851 Exhibition.

It is the property of Mr Grant, of Elchies, Morayshire; - the focal length is 16 feet, and aperture 11 inches: the mounting on the German plan, is by Ransome & May, of Ipswich. The declination and polar axes are about 5 feet long and six inches in diameter; the circles are discs of gun metal, 30 inches in diameter and one inch thick. One portion of the stand consists of 1 tons of iron, the greatest quantity ever cast into a single piece for any astronomical instrument.

The climate of Great Britain very unfavourable to the performance of large telescopes of this character: in the ‘Monthly Notices’ of March 1oth 1854, Mr Grant gives two drawings of Mars, one which, taken with a five feet telescope in India, he says is “actually a little world”, - that taken with the great telescope described above is not nearly so distinct in details,- and he adds, “ I doubt whether the large glass would show it equally well, even were the weather favourable”.

Professor C P Smyth, who made several observations with the Elchies Equatorial last September says, “there were only two occasions during the week when I had the good fortune to witness, for a few minutes each time, a cessation of those atmospheric disturbances on the which the definition of stars seen in a good telescope so greatly depends.” This is but proof, that an instrument of moderate size is more generally useful in this country than one of excessive proportions.


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Friday, 18 September 2026

Cooke Telescope Tales - Cookes and the Mayflower 2

Scientific Instruments made by the York based company Cooke Troughton and Simms which was formed in 1922 were sent across the Atlantic Ocean on board the Mayflower 2.

 The Mayflower 2 sailed on April 20th 1957 from Plymouth in Devon replicating the original voyage of the Mayflower in 1620. The Mayflower 2  arrived in Plymouth Massachusetts on June 22nd 1957 and was then towed to New York City on July 1st 1957.

 The instruments were placed in a treasure chest where when it arrived in New York City was greeted by President Eisenhower. It then became a tourist attraction with its treasures including the Cooke Troughton and Simms instruments being seen by tourists.

 The instruments which were inscribed to commemorate their method of transport will eventually be taken by the company’s representatives in the cities of Boston, Chicago, and the states of California and Colorado.


                                                      www.theramblingastronomer.co.uk

 

Thursday, 17 September 2026

A little ramble through Pegasus the Flying Horse

 The winged horse of Greek mythology, born from the blood of Medusa after she was slain by Perseus, who can be found nearby in the sky.

The most famous feature is the great square outlined by 4 stars. Strangely and for some unknown reason the top left-hand star of the square which used to be known as delta Pegasi has now been transferred to Andromeda where it has become alpha Andromedae.

To the Arab astronomers the square of Pegasus was known as Al Dalw or the Water Bucket

The great square which covers a large area and contains surprisingly few naked eye stars, look at the square you will do well to see a dozen stars.


Alpha or Markab which means Saddle is the bottom right-hand star of the square  its magnitude is 2.5 but is believed to be variable, it is an A class star with a temperature of 9,500’C and is 133 light years away.

Beta or Scheat which means Shoulder is the top right-hand star of the square it varies in brightness between magnitude 2.4-2.7. It is a red M class giant star with a temperature of 3,500’C. The star is 196 light years away.

Gamma or Algenib which means Wing or Side is the bottom left hand star of the square with a magnitude of 2.8, lying 390 light years away. It is a B class star with a temperature of 20,000’ C

Epsilon or Enif which means Nose is 690 light years away and we see it as at magnitude 2.4, it’s an orange K class supergiant star with a temperature of 3,500’C.

Eta or Matar which means Lucky Star of Rain has a magnitude of 2.9 lying 167 light years away. It is a G class giant star with a temperature of 4,700’C.

For a large constellation Pegasus contains few nebulae or clusters, the only object that will interest us is M15 an outstandingly bright globular cluster at magnitude 6.2 which can easily be seen through binoculars. M15 at 12 billion years old it is one of the oldest known. M15 is about 33,600 light years away and is about 175 light years in diameter and contains around 100,000 stars.


                                                     www.theramblingastronomer.co.uk

Wednesday, 16 September 2026

A little ramble through 19th century astronomy - Mu Dorado

Nature November 2nd 1876

Mu Doradus

This star, which was called a fifth magnitude by Lacaille at the end of 1751, and a sixth by Brisbane was observed by Moesta from February 1860 to January 1861 of 8.9m or 9m only.

Perhaps one of our southern readers will put upon record the actual magnitude of this star, the period of which as Moesta remarked would appear to be one of considerable length.


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Tuesday, 15 September 2026

A little ramble through 19th century astronomy - gamma Centaurus in 1857

 Nature June 15th 1876

The double star gamma Centauri

Will one of our southern readers put upon record the actual angle of position and distance of this object, to decide upon the direction and amount of motion which at present are by no means obvious?

Capt. Jacobs’ measures in December 1857 showed that the star was widening as compared to his estimates in March of the preceding year, but he found a retrograde change of angle to the amount of 7 degrees, whereas the angle of 1856 compared with Sir John Herschel’s measures of 1835-36, rather point to direct motion.

Capt. Jacobs says in 1857, “Has opened sensibly since 1853, being now an easy object, whereas then under the most favourable circumstances it could only just be discerned as not round”


                                                     www.theramblingastronomer.co.uk

Monday, 14 September 2026

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE 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 Tales - comet photographed from Ceylon in 1901

The comet of 1901 was photographed by Captain P B Molesworth at the Tricomali observatory in Ceylon (now Sri Lanka)  on May 13th 1901 using a Cooke & Sons camera lens of 8.42 inch focal length. 

The comet had three tails, two slightly diverging, separated by a dark streak; the third is peculiar, as it does not diverge from the nucleus but from a point just behind it. The comet is moving  daily two degrees E N E and has caused quire a sensation among the locals. 

Molesworth was using Klein’s Star Atlas to plot the course of the comet. 

MY NOTE 

This is comet Viscara, which was discovered in Uruguay on April 12th 1901 as a naked eye comet and at its brightest it reached magnitude 1.0. This comet was a southern hemisphere object. It faded from naked eye view on May 20th but was visible in telescopes through until October 1901.


                                                       www.theramblingastronomer.co.uk

Sunday, 13 September 2026

A little ramble through Pavonis the Peacock

 Introduced by Johann Bayer in 1603 it is one of a series of celestial birds in this region of the sky including Apus, Grus, Phoenix and Tucana. The constellation cannot be seen from Britain as it is located close to the south pole star.

In mythology the peacock was sacred to Juno, goddess of the heavens. According to legend Juno sent a creature with 100 eyes called Argus to watch over a white heifer; Juno guessed that this heifer was the form into which her husband Jupiter had turned one of illicit lovers the nymph Io.

At Jupiter’s request Mercury decapitated the watchful Argus and released the heifer. Juno place the 100 eyes of Argus on the peacock’s tail.

The Chinese also saw the constellation as a peacock and called it Joo Tseo

Alpha also known as peacock magnitude 1.9 and is a B class star  with a surface temperature of 17,000’C lying at a distance 179 light years.

The second brightest star is Beta with a magnitude of 3.4  and is an A class star with a temperature of 8,000’C and is 135 light years away.

NGC 6752 a globular cluster. It is the third brightest in the sky, with a magnitude of 5.4 after Omega Centauri and 47 Tucanae, NGC 6752 was first identified by one James Dunlop of Parramatta, Australia on 30 June 1826, who described it as an irregular bright nebula which could be resolved into a cluster of many stars, highly compressed at the centre. This corresponds with a core region densely populated with stars around 1.3 light-years in diameter,


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Saturday, 12 September 2026

A little ramble through 19th century astronomy - new camera equipment in France in 1876

 Nature October 12th 1876

Dr Janssen is devising construction of an automatic photographic revolver, which will take a photograph of the Sun every hour each day of the year from sunrise to sunset. The photographs which will be taken under cloudy conditions, will be useless so far as sunspots are concerned, but they might be utilised for meteorological purposes.

The others will be kept and tabulated. The advantage of this plan it will dispense with any observer and will obtain a mechanical regularity.  A communication will be made very shortly to the Academy of Sciences on the invention which was suggested by the discussion on the Transit of Venus.

It will be set to work in the physical observatory of Dr Janssen.


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Friday, 11 September 2026

Cooke telescope Tales - comet Halley photographed from Egypt in 1910

 On January 24th, 25th, 27th and 28th 1910 Halley’s Comet was photographed by Mr Knox-Shaw at the Helwan observatory in Egypt using a 4 inch Thomas Cooke & Sons telescope. The photographs showed the twin tails and southerly secondary tail.

 The Cooke telescope was attached to a 30 inch reflector that had been purchased in 1902, the reflector was made by A A Common.


                                                       www.theramblingastronomer.co.uk

Thursday, 10 September 2026

A little ramble through 19th century astronomy - meteor seen over France in 1876

 Nature October 5th 1876

Observations have been published by several French provincial papers on the meteor of September 24th. One of the most accurate was in the Echo du Nord  published at Lille. The apparent diameter of the meteor has been stated to have been equal to the Moon in opposition; The same measure was given by M Mamberger, the member for Dunkirk, as reported by that gentleman in a letter to M Leverrier.

The position of the meteor was below Ursa Major, on the eastern side at 20 degrees from the horizon for Lille. The time in Dunkirk and Lille was the same, 6h and 40 m local time, Dunkirk being a few minutes behind owing to the western longitude. The colour was almost the same having been described as reddish blue at Dunkirk and reddish violet at Lille.

A surgeon at Dunkirk said he heard a hissing sound; a sound was also heard at Lille b y a number of people. It was an explosion according to ear witnesses and took place three minutes before the appearance. If correct the observation s shows a distance of about 60 kilometres.

M. Leverrier is collecting and examining statements before entering into a calculation. The light was seen by him at the observatory, as reported before the French Academy of Sciences on the following day. It was seen by a number of persons in Paris. The cloud of burning matter and ashes was observed for a considerable time -0 at least fifteen minutes.


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Wednesday, 9 September 2026

Cooke Telescope Tales - 1898 solar eclipse observed in India

 Total Solar Eclipse, January 22nd 1898 English Preparations by Edward Maunder FRAS 

The English astronomers observed the January 22nd 1898 eclipse of the Sun from various sites. The telescopes  are all achromatic Cooke lenses of 4.5 inch aperture, 5 feet 10 inches focus, and a single quartz lens of 5 inch aperture, 4 feet 9 inches focus   

The third station at Wardha, on the Great Indian Peninsula Railway from Bombay to Nagpur, will be occupied by Mr Newall, who proposes to use a large spilt spectroscope, with two prisms of 62 degrees, in the attempt to determine the speed of rotation of the corona by the relative displacements of its lines as observed east and west of the Sun. 

In the same neighbourhood, Captain Hills will probably fix his apparatus, which will consist of two slit spectroscopes, having the slit tangential to the Sun’s limb at the point of second contact and diametral receptively. The slits are 1.5 x 0.004 inches and 2 x 0.004 inches respectively; and the prisms are, for the first spectroscope, of two flint prisms of 60 degrees, 4.5 inch base, 2.5 inch height at maximum deviation for Hydrogen gamma and for the second spectroscope, of four quartz prisms of 60 degrees, 3.25 inch base, 2.75 inch height at maximum deviation for Hydrogen epsilon. The collimator and camera lenses are single quartz lenses, of 2.5 inch aperture , 30 inch focus and 3 inch aperture and 36 inch focus.


                                                     www.theramblingastronomer.co.uk

 

 

Tuesday, 8 September 2026

A little ramble through 19th century astronomy - diameter of Vesta in 1876

 Nature September 28th 1876

At the opposition of 1855, this brightest of the minor planet group, which during the last spring, as in previous favourable oppositions, was discernible to the naked eye, was observed by Prof Secchi to present a diameter but little inferior to that of the first satellite of Jupiter and he estimated it at 0.8 seconds; this we find corresponds to a true diameter of 450 m lies.


                                                         www.theramblingastronomer.co.uk

Monday, 7 September 2026

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE 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.

 

A little ramble through Orion the Hunter

Without doubt the brightest and grandest constellation in the sky.

In one Greek story Orion was boasting to a large crowd of people of all the animals he had killed, however he did not see a scorpion creeping up behind him. The scorpion stung him on the ankle and killed him. The gods were so impressed with his boasting that he was placed in the sky forever. So was the clever scorpion. To make sure they could never meet again Orion was placed in the winter sky while the scorpion was placed in the summer sky.

In Egypt Orion was seen as Horus in a boat surrounded by stars while the Arabs saw Orion as Al Jabbar the Giant or Al Babadur the Strong One.

In Hindu astronomy Orion was seen as Praja-pati seen chasing his daughter across the sky, the daughter being Aldebaran the brightest star in Taurus. In China Orion was the White Tiger.

The Anglo Saxons called it Ebuorung referring to the Milky Way, while the Vikings called the constellation Goddess Frigg or Mother Earth.

Alpha Orion of Betelgeuse which means The Armpit of the Central One. Most other astronomers from various civilisations refer to Betelgeuse as an Arm. Betelgeuse is the star that some people like to refer to as Beetlejuice.

Betelgeuse is the 9th brightest star in the sky. It varies in brightness between 0.4-1.3 these variations were first reported in 1836 by John Herschel, the son of William Herschel who discovered the planet Uranus in 1781.  When at its faintest it is decidedly fainter than Rigel. During the winter of 2019-2020 Betelgeuse became very faint causing astronomers to wonder if it was in the process of going supernova. It wasn’t, Betelgeuse produced a massive flare that blocked some of the light from the star.  The star has in fact been as faint as this before in 1927. It is a red supergiant star entering its final phase and will probably go supernova within the next 1 million years.   It is 642 light years away and is a M class supergiant with a temperature of around 3,300’ C.

Beta or Rigel is usually referred to as The Left Foot of the Giant, however the Arab astronomer Al Sufi in his star catalogue called it Rai al Jauzah or The Herdsman of the Camels. Rigel is the 7th brightest star in the sky at mag 0.1. It is 863 light years away and is a B class supergiant star with a temperature of around 12,000’ C and like Betelgeuse will end up going supernova.

Gamma or Bellatrix which means the conqueror or Amazon star is the 3rd brightest star in Orion. Al Sufi referred to the star as Al Ruzam or the Lion.  It has a magnitude of 1.6 and lies at 250 light years. It is a B class giant with a temperature of 21,500’ C.

There is a Harry potter connection with Bellatrix because one of the characters form the Harry potter stories is Bellatrix Lestrange. I think she was one of the baddies.

Orion’s Belt is formed of three stars and from left to right they are;

Zeta or Alnitak which means the Girdle is the left-hand star of the belt. Alnitak has a magnitude of 2.0 and is 1200 light years distant. It is one of the rare O class supergiant stars with a temperature of 29,000’C. Alnitak will become a supernova in the future

Epsilon or Alnilam which means String of Pearls at magnitude 1.6 is the 4th brightest star in Orion. Alnilam is the middle star of the belt. Its distance is about 2,000 light years, and is a B class supergiant with a temperature of 27,000’C. It will also go supernova in the future.

Delta or Mintaka the right-hand star of the belt its name means the Belt, its magnitude is 2.2 and also lies 1200 light years away, another of the rare O class stars with a temperature of 29,000’C, and as with Alnitak, Mintaka will become a supernova.

Kappa or Saiph which means The Right Leg of the Giant is of magnitude 2.1 and lies 650 light years away, it is a B class star with a temperature of 26,000’C.

Iota or Na’ir al Saif, which means "the Bright One of the Sword is the brightest star in the asterism known as the sword of Orion, magnitude 2.8 and lying at a distance of 2,300 light years. Like many of the stars in Orion it is one of the rare O class giant stars with a temperature of 32,000’C. As with the O class stars in Orion, it will become a supernova in the future.

Messier 42/43

Below the stars that form Orion’s Belt is the Orion Nebula, an area of the galaxy where stars are being formed.

One of the great mysteries in visual astronomy is that Galileo apparently never noticed the great nebula in Orion. There also appears to be no record of it in medieval records either. Yet here is one of the grandest naked eye nebulae in the heavens just below the famous Orion belt stars. It could not possibly have been missed by Galileo and is especially puzzling. It is also interesting that the Arab astronomers including Al Sufi had recorded the much fainter nebula in Andromeda M31 but not the Orion nebula. What could have been going on? The first mention in western records is around 1615.

There are hundreds of stars being formed here today. The Orion nebula is an enormous cloud of gas about 40 light years in diameter. The cloud is illuminated by a group of four stars known as the Trapezium, these four jewels are between magnitude 5 to 8, all the stars which are very young being about 1 million years old and there are thousands of unseen stars between 300,000 to 1 million years old. The nebula is about 1600 light years away.

M43 is a separate nebula often overlooked because of its close proximity to the Great Orion Nebula, it is separated from M42 by a dark lane of gas known as the Fish Mouth. M43 surrounds a 7th magnitude star known as Bond’s star. To see M43 you have to block the light from M42. 

M78

A diffuse nebula with a magnitude 8.3 and lying at a distance of 1,300 light years, above and to the right of the star Alnitak. You would need a pair of binoculars just to glimpse it.

Surrounding Orion is the Barnard Loop, this is the remains of a supernova that exploded about 2 million years ago. It was first photographed by Edward Barnard in 1883; it can be seen with the eye under the best of conditions. There are suggestions that it was seen by the Vikings over 1,000 years ago.


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Sunday, 6 September 2026

Cooke Telescope Tales - astronomy photographs taken in 1853

Some of the early astronomical photographs were taken in England by astronomers using Thomas Cooke & Sons telescopes.

 In 1853 John Phillips in the Museum Gardens in York using a 6.25 inch telescope photographed the Moon. In 1857 Mr Fry using Mr Howell’s 6.5 inch telescope in Brighton were amongst the first astrophotographers. 

At this period of time telescopes were designed for visual use and all the gentlemen astronomers had the problem using refractors of the difference between the actinic and visual foci. Reflecting telescopes did not suffer from such problems. 

The negatives obtained by both Phillips and Fry were about 1 inch in diameter.


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Saturday, 5 September 2026

A little ramble through 19th century astronomy - telescope lens in France in 1876

 Nature September 14th 1876

The council of the Paris Observatory has resolved to attempt the manufacture of object glasses by machinery instead of by hand. The mechanical cutting of flint and crown glass will be executed by M Lessautre, the well known clock maker, who prepares the optical part of the French lighthouses by machinery.


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Friday, 4 September 2026

Cooke Telescope Tales - The Universal Exhibition in Paris in 1855

The last French Monarch of France Napoleon III who was nephew to the Emperor Napoleon was rebuilding Paris in 1855 and wanted he Exposition of that year to be the most impressive. The Paris Expositions were begun in 1789. 

Although Napoleon wanted it to be the greatest art and industrial event ever staged it had already been eclipsed by the Great Exhibition at Crystal Palace in Britain in 1851. The exposition would run from June to November 1855. 

This exhibition allowed Cooke to become known in Europe. Among the exhibitors was Thomas Cooke of York who took the brave step of exhibiting a variety of optical equipment including a 7.5 inch equatorial with a clock work drive. 

Cooke was exhibitor No. 392 and was described as selling astronomical and nautical instruments. He was in the 8th section ‘Arts connected with Science and Education’. 

For Cooke it was a great success not only because he won a First Class Medal for his 7.5 inch telescope he also made some very good contacts including the astronomer Warren De La Rue. 

He also met Lt Gen Edward Sabine, astronomer, geophysicist and explorer and Lt Col Strange from the East India Company, the latter two would be very important in ensuring that Cooke theodolites being used in the great survey of India. 

He also introduced himself to the astronomers of Europe and in the following years there would be orders for telescopes and observatories from countries such as Austria, Belgium, Denmark, Hungary, Italy, Russia and Sweden.


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Thursday, 3 September 2026

A little ramble through 19th century astronomy - new nebulae in 1876

 Nature August 17th 1876

M Stephan, Director of the Observatory at Marseilles, has communicated to the Pars Academy a list of twenty-three new nebulae detected with the Foucault telescope of 0.80m, aperture, which raises the number of such discoveries, so far published to 120; but M Stephan mentions that he has approximately positions of about 400 new nebulae.

As might be expected the twenty-three new nebulae are mostly very faint;


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Wednesday, 2 September 2026

Cooke Telescope Tales - telescope for Eton in 1870

In 1870 one of the masters possible H G Madan at Eton School decided that they would provide a telescope. They chose a 5.9 in Thomas Cooke & Sons Refractor. The observatory was also made by Cookes. The observatory was erected on the roof of the western tower of the New Schools. It is square and surmounted by a revolving dome. 

Although a telescope on a roof will never be completely free from vibration it is reduced to a minimum by supporting the telescope on two massive trussed iron girders stretching across the observatory. The floor is supported quite independently. 

The telescope which was up the normal Cooke standards was supplied with the new Cooke clockwork driving system which was designed by the late Thomas Cooke.

 The science master at Eton School was  H G Madan who was the brother of Falconer Madan who was himself the grandfather of Venetia Burney who suggested the name Pluto for that newly discovered planet in 1930. 

I believe that the Eton telescope is still in use today in a different observatory located next to Eton Golf Course and is used by the Herschel Astronomical Society.


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Tuesday, 1 September 2026

A little ramble through Ophiuchus the Serpent Bearer

Ophiuchus is one of three large constellations visible in the summer months in the southern part of the sky, the others being Hercules and Serpens which are all formed of faint stars.

Ophiuchus is an ancient constellation depicting an elderly  man encoiled by a serpent. In the night sky today, Ophiuchus clearly had the best of the struggle with the serpent as it is n ow depicted in two halves one being the body of the serpent the other being its head.

 He is identified to the Greeks as a mythological forerunner of Hippocrates who served as the ship’s surgeon aboard the ship the Argo., with Jason looking for the golden fleece.

It was said the medical work of Ophiuchus was so great he could bring the dead back to life. He tried but failed to b ring Orion back to life after he had been stung by a scorpion. 

In Rome, Pliny considered that the stars that formed Ophiuchus were dangerous to mankind through the killing of people by poisoning.

The brightest star alpha is known as Rasalhague which means ‘Head of the Serpent Charmer’ it has a magnitude of mag 2.1 and is an A class giant star with a surface temperature 7,500’C which is much hotter than the Sun. Rasalhague is 47 light years away.

Eta or to the Arabs Saik or the Driver is of magnitude 2.4 and is 88 light years away. It is an A class  star with a temperature of 9,600’C

Beta or Alrai which means The heart of the Shepherd is a magnitude mag 2.8 star lying 82 light years away. Alrai is a K class giant star with a surface temperature of 4,100’C.

Delta or Yed Prior which means ‘Hand’ is of magnitude 2.8 and is a M class red giant with a temperature of 3,400’C lying at 171 light years away. In China the star is known as Leang or Mast.

In 1604 Johannes Kepler saw a supernova in Ophiuchus, a supernova is a star that destroys itself in a massive explosion.  the last easily This was the last bright supernova to be seen in our galaxy. It reached a magnitude of -2.1 and was visible to the naked eye for around 18 months. This was before the first use of the telescope for astronomical uses which was in 1609.

Probably the most famous star in Ophiuchus is one that cannot be seen without binoculars or telescopes this is Barnard’s star a 9th magnitude star only 6.1 light years away, the fourth closest to the Sun after the 3 stars in the alpha centauri group. It was found by Edward Emmerson Barnard in 1916. It is a red dwarf star.

There are a large number of Messier objects in Ophiuchus

 

Messier 9

Globular cluster discovered in 1764 mag 9.3 one of the closer globular at a distance of 5,500 light years.

Messier 10

Globular mag 6.4 discovered in 1764 diameter of 83 light years 13,400 light years

Messier 12

Globular discovered in 1764 15,700 light years away mag 7.7 diameter 75 light years

Messier 14

Globular cluster mag 7.6 30,000 light years away and 100 light years across

Messier 19

Globular cluster discovered in 1764 mag 7.5 28,000light years across

Messier 62

Globular cluster discovered in 1771 magnitude 6.4 and 22,000 light years away

Messier 107

Globular cluster probably seen by Messier in 1782 and is 21,000 light years away and is of magnitude 8.9

The following are not in the |Messier list

IC 4665 

An open cluster at mag 4.2 visible to naked eye, also binoculars or small telescope. For some reason it was not catalogued by messier it lies at 1,400 light years away and is about 40 million years old.

NGC 6633

Open cluster mag 4.6 again not catalogued by Messier it contains about 30 stars and is around 660 million years old.

Although not classified as a zodiacal constellation Ophiuchus does lie in the zodiac. It can be found between the constellations of Sagittarius and Scorpio. This means that there are times when planets can be found passing through Ophiuchus.


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