Saturday, 31 May 2025

Professor Bond, and the Orion Nebula in 1863

 It is understood that Professor Bond of Cambridge F.S.A, is preparing for publication a lengthy memoir in 1863  on this magnificent object, embodying the results of 14 years observations, latterly made with Alvan Clark’s large object glass of 18.5-inch aperture.

The spiral structure of the nebula which has lately been distinctly visible in this glass and the supposed change of its appearance within the last few years, will doubtless be found amongst the topics treated off.



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Friday, 30 May 2025

A little ramble through Canes Venatici the Hunting Dogs

 Canes Venatici or the Hunting Dogs is a modern constellation, created by the Polish astronomer Johannes Hevelius 1611-1687 who introduced this constellation to the star maps in the 1680s. He introduced 9 new constellations of which 8 are surprisingly still used today.  Although most are faint groups that fit in-between the ancient classical constellations. Canes Venatici is probably one of the brighter examples.

This constellation is what is known as a northern circumpolar constellation. This means that we can see it all year round. It does not matter what season we are in. If we think about Earth in space in a 3-dimensional way, then whichever season we are in we see those stars in the night sky. There are stars in the daytime sky, which we can’t see because the Sun is so bright we can’t see behind it. These stars are from the opposite season. To give an example if we are looking at stars in the autumn the stars that we would see in spring night sky would be in the daytime sky.

However, as we are thinking three dimensionally there will be stars above and below the Earth. These are the circumpolar stars, northern for the northern hemisphere and southern for the southern hemisphere. This means it does not matter where the Earth is in its orbit around the Sun whether it be spring, summer, autumn or winter we will always see the circumpolar stars.


The stars that form Canes Venatici were once part of Ursa Major the Great Bear. They can be found under the handle of the Plough. The Plough is an asterism of 7 stars which is part of a much larger group called Ursa Major or the Great Bear.

 Most civilisations seem to regard that these stars were part of Ursa Major certainly  this was the general belief of the Greek Chinese and Arab astronomers.

According to Greek myths the hunting dogs were being held by Bootes the Herdsman, and it is suggested that this may be to prevent them from chasing the two bears around the sky. There are only two stars of any note in the constellation alpha or Asterion and beta or Chara.

The story now becomes a little confusing because when Hevelius created the constellation Asterion which means Starry changed its name to Cor Caroli which is still used today. Cor Caroli means Charles’ Heart. Some sources suggest it was named in honour of King Charles I who was executed in 1649 while some suggest that it was named in honour of King Charles II when he became king in 1660. It has been suggested that it shone brightly when he returned to England.

The Chinese regarded Asterion and two faint nearby stars as San Kung, the Three Honorary Guardians of the heir Apparent. However, the Arab astronomers saw an extra faint star in this group and called it Al Karb al Ibl, The Camel’s Burden.

Cor Caroli itself is a star with a magnitude of 2.9 lying at 110 light years. It varies slightly in brightness and is the prototype star for the alpha Canes Venatici type variable stars. It’s an A class star meaning that it is hotter than the Sun

Just to keep the confusion going beta or Chara which means the Southern Dog is the name that is still used today.  Chara is a fainter magnitude 4.3 star lying at a distance of 27 light years and it’s a G class star slightly hotter than our Sun.

There is one variable star I would like to mention and that is Y Canes Venatici or to give it its name La Superba. It varies in brightness between magnitudes 4.3 to 7.8 so at its brightest it can be seen with the naked eye but when it is at its faintest a pair of binoculars will be need to see.it.

Astronomers refer to this star as a  semi regular variable star reaching its brightest every 160 or so days.

It is known as La Superba because it is one of a rare group of stars that astronomers refer to as carbon stars, these are stars very close to the end of their lives, La Superba only has a temperature of around 2,700 degrees making it one of the coolest known true stars. La Superba lies at about 1,000 light years away and is in the process of becoming a planetary nebula leaving behind its core which is a white dwarf. This is the eventual fate of our own Sun.

The name La Superba was given to the star in 1866 by the Italian Catholic Priest astronomer Father Secchi 1818 – 1878 due to its very deep red colour.

There are no less than 5 messier objects in Canes Venatici.

M3

 Oddly enough, when Charles Messier first noticed this object on May 3rd, 1764, it was only the 76th Deep Sky Object ever seen by human eyes (with the assistance of telescopes, that is). Although Messier had logged his previous two discoveries M1 The Crab Nebula and the globular cluster M2 it was this third object that prompted him to begin his now famous catalogue of ‘objects that are not comets’.

Messier Object 3 a globular cluster. Since it was first observed, this globular star cluster has gone on to become one of the best-studied objects in the night sky and is considered by many amateur astronomers to be one of the finest visible clusters.

Globular clusters are densely packed collections of ancient stars. Roughly spherical in shape, they contain hundreds of thousands, and sometimes millions, of stars.

M3 is one of the largest and brightest and most splendid star clusters and is made up of around 500,000 stars. It is located at about 33,900 light-years from Earth, the cluster spans about 220 light-years. It is estimated to be 8 billion years old, making M3 one of the oldest formations in our galaxy. It has a magnitude of 6.2 which means it is invisible to the naked eye, a pair of binoculars would be needed to find it.

M51

The famous Whirlpool Galaxy. Once believed to be a great swirling nebula in our galaxy M51 is now known to be the finest example of a face on spiral galaxy. A near neighbour at only 15 million light years away this graceful pinwheel of stars and gas is about 500,000 light years across. Binoculars are needed to find it as it has a magnitude of 8.4.

Lord Rosse in Ireland at Birr Castle in 1845 used his 72-inch telescope which at the time was the largest telescope in the world to study M51, he was the first person to see the spiral structure with the stars. Some astronomers of the time after seeing these drawings believed that M51 was a stellar universe like the one in which we live. This was of course based on knowledge of the day; astronomers didn’t realise that there are billions of other galaxies they assumed that our galaxy was the universe.

There is a small satellite galaxy located at the end of one of its spiral arms.

Messier discovered M51 in 1773 and described it a s a nebula without stars near the northerly ear of Canes Venatici below the second magnitude star (Eta end star) in the tail of Uma. He said it was only seen with difficulty with his simple telescope.

M63

The Sunflower Galaxy in photographs looks like a spiral galaxy that has lost control of its gravity, and we are catching a rare sight of its arms being tossed into space.

This spiral galaxy is a prime example of a type of galaxy that displays a lack of cohesion between its inner and outer arms The inner region of M63's is 86,000 light year wide disk is ringed by a strong spiral structure and the plentiful outer arms appear loose, patchy and haphazard. Not surprisingly M63 is nicknamed the Sunflower Galaxy because of its resemblance to that towering plant whose dense seedy head is ringed with an abundance of bright overlapping petals. M63 lies at around 29 million light years and at magnitude 8.6 is below naked eye visibility and can be seen by binoculars or small telescopes

Charles Messier observed M63 on June 14th, 1779, who described it as faint and does not contain any stars. It is close to a 8th mag star.

M94

The Croc’s Eye Galaxy despite its placid appearance, may have experienced an explosion only 10 million years ago, a cleansing event that disgorged millions of solar masses of material out of its disk or nucleus. The galaxy lies at 16 million light years and has a magnitude of 8.2.

Messier observed M94 in 1781 as a nebula without a star above Cor Caroli. The centre is bright and the nebulosity not very diffuse.

M106

Another spiral galaxy this time it does not appear to have a name. It looks like M94 and appears odd shaped suggesting that it also survived some violent upheavals in the past. Like most galaxies we see there appears to be a black hole at its centre, this was discovered in 1994.

Lying at 22 million lights and shinning at magnitude 8.3 it can be just seen through binoculars as a faint spot but really binoculars will be needed to see it.

Messier leaves no notes to this galaxy.


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Thursday, 29 May 2025

Northern Lights and a meteor seen in March 1863

A brilliant display of this phenomenon was seen by Mr E J Lowe of Beeston Nottinghamshire on the evening of the March 21st, 1863, shortly after eight o’clock it reached an altitude of 43 degrees. 

At 8.33 a meteor first equal to a fourth but increasing in size to a star of the first magnitude, passed from zeta Perseus to alpha Aries, becoming remarkedly red when passing through the Aurora.



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Wednesday, 28 May 2025

The Elchies Telescope made by Mr Ross and shown at the Great Exhibition of 1851

In the number of the ‘Monthly Notices’ for November 1862, 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 10th 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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Tuesday, 27 May 2025

The 74 inch telescope at the 1951 Festival of Britain

 The 1951 festival of Britain a national exhibition that was visited by millions of people during the summer of 1951.


                                    The 74 inch telescope at the 1951 Festival of Britain exhibition 

Among the many futuristic displays was the 74 inch telescope built by Grubb Parsons of Newcastle, after the festival it was sent to the Mount Stromlo Observatory in Australia where sadly it was destroyed by a bush fire during 2003.

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Monday, 26 May 2025

Leeds Observatory in 1906

 Leeds Mercury Saturday 27th January 1906.

One the old stone houses on the Woodhouse Moor Reservoir at the Grammar School side has been adapted for astronomical use and a large 18-inch reflector telescope has been placed in position there. This telescope is the gift of Major Duncombe, and is fitted with the customary mounting, range-finding, and clockwork appliances. In an adjoining room a transit instrument has been mounted, and this, like the telescope, is now almost completely adjusted for use. The dome of aluminium is moveable, and apertures may be opened to suit the convenience of the astronomer.



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Sunday, 25 May 2025

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.

Venus visible in dayight in 1902

 Yorkshire Post and Leeds Intelligencer Wednesday 15th January 1902

 To the Editor of the Yorkshire Post. 

Sir, Shakespeare’s ‘bright star of Venus’ forms so conspicuous an object in the evening south western sky that one led to inquire if she has been seen in the day time with the naked eye during her present effulgence. Perhaps some local astronomer has observed her through the atmosphere of ‘dim, laborious Leeds; Mr Whitemell, it may be.

 To a great many people the fact that a star can be visible at noon day at all must border on the incredible, bit Venus is not infrequently detected, though  ore by accident than by design to the un astronomical.

 The late Mr Edwin Dunkin, who for nearly half a century was with the Royal Observatory at Greenwich wrote:- ‘ At the times of greatest brilliance the light Venus is very intense. A sensible shadow is often thrown upon a piece of white paper the interposition of the hand between it and Venus when the planet is in this position in its orbit. It can almost be plainly perceived by naked eye at such times in full sunlight, sometimes within an hour of noon. At one of these epochs in 1868, a correspondent of the The Times fancied that he had discovered a balloon shaped comet at noon day by means of a small telescope. The stranger, however turned out to the the planet Venus, which happened to be favourably situated for daylight observation in the spring of that year.

 Sir Robert Ball, too refers the subject in his ‘Story of the Heavens’, thus:- ‘When Venus is at its brightest it easily can be seen in broad daylight with the unaided eye. This striking spectacle proclaims in unmistakeable manner the unrivalled supremacy of Venus compared with the other planets and the fixed stars. Indeed, this time Venus is from 40 tom 60 times as bright as the brightest star in the northern heavens’. But of course a desire for star finding in the day time is to know where to look for your star.

 

J H Elgie 

Leeds, January 14th



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Saturday, 24 May 2025

A little ramble through 19th century astronomy - Changes observed on Jupiter in 1869 by John Browning

During the months of October and November 1869 the planet Jupiter has presented a spectacle of singular and almost exampled beauty. The belts on the planet are more than usually numerous, and they display a greater variety of colours than I have ever yet seen ascribed to them. The equatorial belt, which has been for years the brightest part of the planet is now not nearly so bright as the light belts to the north and south; usually it has been free from markings, and now it is often covered with markings, which resemble piled up cumulus clouds: it has generally been colourless, shining with a silver grey or pearly lustre – now it is a rich deep yellow, greatly resembling the cloud of electotyped gold.

The woodcut represents Jupiter as it was seen on the night of 9th October 1869 in a reflecting telescope with a silvered glass mirror of 12.25 inches diameter. The upper part of the planet is the South Pole. On this portion of the disc there are three dark belts, while on the North Pole there are only two.

The poles of the planet are ashy blue, and the darker belts nearest to them present a darker tint of the same colour. The bright belts next, these are pearly white, and shine more brilliantly than any other portion of the planet. The dark belts next to the central bright belts are coppery red. As already mentioned, the central belt, which has been for many years a pearly white, is now a rich golden yellow.

Three of four dark markings on the lower part of the southern dark belt nearest the equator will be seen to incline to the left. If our Earth were removed to Jupiter’s distance, its disc would appear no larger than these dark masses, so enormous is their extent. The rotation of the planet is carrying them towards the right: we may assume that the bright vapour between them is left behind by the planet, which is here travelling at the rate of nearly 3,000 miles per hour.

Spectrum analysis has taught us to respect that any change in the colour of the light proceeding from an object, indicates a change of the object itself. If Jupiter, the largest planet in the solar system has still retained so much heat as to shine partially by its own light, the present considerable change in colour may enable spectroscopist to obtain some information on this interesting subject.

John Browning



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Friday, 23 May 2025

A little ramble through Cancer the Crab

 Cancer is a zodiacal constellation in fact it is the faintest of the constellations that can be found in the zodiac. It can be found in the sky between Gemini the Twins and Leo the Lion both more spectacular examples of constellations in the zodiac.

The zodiac is an area of sky where all the planets in the solar system can be found. The name zodiac dates to around 300 BCE and was given by Greek and Roman astronomers, it means the little ring of animals. Libra is not an animal and was added later around 50 BCE when part of the constellation was hived off to form the constellation of Libra the Scales. The zodiac was known by the Babylonian astronomers of around 4,000 years ago which referred to this area of the sky at the Mirzata which means The Watch.

The constellation can best be described as looking like a ghostly version of Orion the Hunter. In mythology Cancer represents a crab that Juno queen of the gods sent to battle Hercules who was fighting the mufti headed monster. The crab did not affect the outcome because Hercules killed the monster and simply trod on the crab. However, as a reward for the efforts of the crab it was placed in the sky for ever by the gods.

The Akkadians who had an empire which existed from about 2240 BCE to 2284 BCE described Cancer as the Sun of the South, perhaps due to the position of the constellation during the winter solstice many thousands of years ago.

The Persians called the constellation Kalakang, the Chaldeans called it Sartono and the Arabs called it Al Saratan, all these names refer to Cancer. In Babylon it was a turtle and around the 1000 CE the Saxons called Cancer Crabba.

As I mentioned it is a very faint constellation the brightest star is beta with a magnitude of only 3.5 it lies 390 light years away and is a class  K class giant star cooler than our Sun. Bea is called Al Tarf which means the end of the southern foot.

Alpha is called Acubens which means the claw it’s  a magnitude 4.3 A class star and it is hotter than our Sun. It lies at a distance of 178 light years.

Iota is a binary star the fainter star cannot be seen without the use of a telescope. The main star has a magnitude of 4.0 and is a G class giant star and is 320 light years away.

The last two stars I want to mention are not very bright, but they play a part in a very interesting story. The stars are gamma with a magnitude of 4.7 and delta with a magnitude of 3.9. Gamma is known as Asellus Borealis of the Northern Donkey and delta is called Asellus Australis the Southern Donkey they are either side of the open cluster M44 or Praesepe the Beehive Cluster.

The letter M signifies that it is on the list of messier objects catalogue by the French astronomer Charles Messier during the 18th century on his quest to discover comets.

The term the Beehive appears to have been first used by Admiral William Smythe during the 1840s when he described it as looking like a swarm of bees. The cluster is a naked eye object it observed by Hipparchus around 2,200 years ago who described it as a Little Cloud. It was one of the first objects that Galileo looked at through his new telescope he counted around 40 stars. Today we know there are over 1,000 stars there. The cluster lies at a distance of 590 light years.

However, there is another older name for the beehive and that is the Manger, which is a vessel that animals would have eaten out of. According to some classical Greek myths and legend Greek heroes charged into battle riding donkeys because the Titans were scared of the braying noise that the donkeys made. For this good service two donkeys Asellus Australis and Asellus Borealis were placed into the sky next to the manger to enjoy some food.

The story becomes even more interesting because it appears that around about 2,000 years ago the term the Crib starts to get used to describe the star cluster. Is this some kind of biblical reference celebrating the birth of Jesus?

There is a second messier object M67 which is a smaller open cluster lying 2,600 light years and containing around 200 stars.  At magnitude 6.1 a pair of binoculars will be needed to see it. It is often the case when there is a particularly famous messier object in a constellation another one can become overlooked, and this is what happens to M67.

One lats piece of information regarding Cancer and I can never resist mentioning it is that Asellus Australis also has a Babylonian name which I believe holds a record for the longest name of a star, Arkushanangarushashutu,  (22 letters)  Try saying that quickly. The name translates to ‘the south-east star in the Crab’. 



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Thursday, 22 May 2025

New comet in 1821

 

Leeds Intelligencer Monday 5th March 1821

 

The Comet. The new comet  Observatory, Gosport, Feb. 24.

 

 A comet made its appearance here last evening at 35 minutes past six o'clock, within two or three degrees of Algenib, the last star in the wing of Pegasus. It is 32 degrees to the east of the sun, and sets with Saturn soon after eight o'clock, about W. N. W. but is 18.5 degrees to the north of that planet. Its small light nucleus was surrounded by a diffused coma, three fourths  of a degree in diameter by the sextant, and its perpendicular tail, was nearly 4 degrees  in length when the coruscations were most vivid, through the upper part of which a small star of the sixth magnitude was perceived by the help of a telescope. This is unquestionably the same comet that Seigneur Pons, Astronomer of the Ductless of Lucca, discovered in the constellation Pegasus, in the evening of thee 21st ult., but which, to our knowledge, has not yet been seen by the English astronomers.

 

 

Leeds Intelligencer Monday 5th March 1821

 

The new comet has been seen at Wakefield, and also at Bingley. Its nucleus is exceedingly brilliant; its tail, which is about four degrees in length, appears larger at the beginning than at the extremity. Its apparent motion is very slow; it has barely proceeded two degrees and a half in right ascension and declension from the 21st of January last, to the 22nd of Feb. It sets about eight o'clock in the evening. The most favourable time for seeing it is, therefore, from six to half-past seven o'clock. It is in the West and still in the constellation of Pegasus. We have not yet heard of its having been observed at Leeds.

 

Note

This was comet Nicolett-Pons (J N Nicolett Royal Observatory Paris and J L Pons Marlia Italy) was discovered on January 21st 1821 near gamma Pegasus, it was at its brightest on March 6th when it was reported at between magnitude 3 to 4.



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Tuesday, 20 May 2025

Telescope in railway lost property in 1867

Sheffield Daily Telegraph Saturday 16th March 1867 

Among the curious things connected with the business of railways are the variety and strange character of the unclaimed property which falls in to the hands of the railways as carriers of passengers and goods. 

One person has left a very superior astronomical telescope in mahogany case complete, and it is now unclaimed. Where is its owner and what has he been doing to render himself unconscious of the loss he has sustained? Or has he abandoned the study of astronomy for the more prosaic and common occupations of the earth?    


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Monday, 19 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.

A little ramble through 19th century astronomy - The Emperor of Brazil was an astronomer

Notes from Nature Magazine

July 20 1871

It perhaps is not so generally known as it ought that the Emperor of Brazil, now in this country is an enthusiastic astronomer, and has an appreciation of the value of science which places him in the highest rank among reigning sovereigns. During last week he has visited the Royal and Mr Huggin’s observatory, and in a long interview with Mr Lockyer has discussed the bearings of the recent solar discoveries.

 

Dom Pedro II (Pedro de Alcântara João Carlos Leopoldo Salvador Bibiano Francisco Xavier de Paula Leocádio Miguel Gabriel Rafael Gonzaga; 2 December 1825 – 5 December 1891), nicknamed the Magnanimous, was the second and last monarch of the Empire of Brazil, reigning for over 58 years.



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Sunday, 18 May 2025

Occultation of Saturn observed from Leeds in 1900

 Yorkshire Post and Leeds Intelligencer Friday 7th September 1900 

 

 To the Editor of The Yorkshire Post. Sir,—

 

This interesting phenomenon was seen here on Monday, 3rd inst. The disappearance took place at the dark east limb of the moon, and lasted about 80 seconds, the west part of the ring, then the planet, then the east part of ring, being successively hidden. The major axis outer ring measured about 40in. The moon, near meridian, had an altitude of some 15 degrees, and was yellowish. Saturn appeared very pale, almost white, in comparison with the moon.

 

The times of  beginning and ending were, approximately,  7h. 12m. 18s., and 71a 13m. 28S, so that the occultation hero occurred earlier than Greenwich, for which place 7h. 16m. was the predicted time for disappearance, and 8h. 11M  for reappearance. The reappearance of the planet the moon’s bright west limb was entirely lost in cloud.

 

The telescope is a 3.25 inch  refractor, and I observed with power of 105.—Yours, etc., C. T. WHITMELL, President Leeds Astronomical Society. Leeds. 6th  September.


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Saturday, 17 May 2025

A notable shoemaker from 1896

 Sheffield Daily Telegraph Tuesday 4th February 1896

On Sunday morning- there was carried to the grave at Darlington Cemetery Mr. W. H. Harris, who was a working shoemaker, living in a poor neighbourhood, at Hank Top, Darlington. Mr. Harris, who was 54 years old the time his death, was born at Barnard Castle. 

Though working hard at his trade, he had attained local celebrity as an astronomer, and maker of telescopes with 9 inch and 12inch mirrors, which he, ground, figured, and silvered. This work required nice mathematical calculations, which he carefully worked out. He had intimate knowledge of optics, botany, astronomy, electricity, etc., and was a good French scholar. Mr. Harris was self-taught.



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Friday, 16 May 2025

A little ramble through 19th century astronomy- On the Great Sunspot of June 1843

 From the ‘American Journal of Science and Arts vol 1 April 1871

On of the largest and most remarkable spots ever seen on the Sun’s disc appeared in June 1843 and continued visible to the naked eye for seven or eight days. The diameter of the spot was according to Schwabe 74,000 miles; so that its area was many times that of the Earth’s surface.

Now it has been observed during a number of sunspot cycles that the larger spots are generally found t or near the epoch of the greatest numbers. The year 1843 was however a minimum epoch of the eleven-year cycle. It would seem therefore, that the formation of this extraordinary spot was an anomaly, and that its origin ought not to be looked for in the general cause of spots of Schwabe’ cycles.

As having a possible bearing on the question under consideration, let us refer to a phenomenon observed at the same moment on the 1st September 1859, by Mr Carrington at Redhill and Mr Hodgson at Highgate. Mr Carrington had directed his telescope to the Sun, and was engaged in observing his spots, when suddenly two intensely luminous bodies bust into view onto its surface. They moved side by side through a space of about thirty-five thousand miles, first increasing in brightness, then fading away. In five minutes, they had vanished… It is a remarkable circumstance that the observations at Kew show that on the very day, and at the very hour and minute of this unexpected and curious phenomenon, a moderate but marked magnetic disturbance took place, and a storm or great disturbance of the magnetic element, occurred four hours after midnight, extending tom the southern hemisphere.

The opinion has been expressed by more than one astronomer that this phenomenon was produced by the fall of meteoric matter upon the surface of the Sun’s surface. Now the fact nay be worthy of note that the comet of 1843, which had the least perihelion distance of any on record, actually grazed the solar atmosphere almost three months before the appearance of the great comet of 1843. The comet’s least distance from the Sun was almost 65,000 miles. Had it approached but little nearer, the resistance of the atmosphere would have probably brought its entire mass to the solar surface. Even at its actual distance it must have produced considerable atmospheric disturbance.

But the recent discovery that a number of comets are associated with meteoric matter, travelling in nearly the same orbits, suggests the inquiry whether an enormous meteorite following in the comet’s train and having a somewhat less perihelion distance may not have been precipitated upon the Sun, thus producing the great disturbance so shortly after the comet’s perihelion passage/

Daniel Kirkwood, Bloomington, Indiana


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Thursday, 15 May 2025

Naked Eye Comet seen in 1819

 

Leeds Intelligencer Monday 12th July 1819

 

THE COMET.

 

The following communication from Mr. Christie of the Royal Military Academy, Woolwich, contains probably all that can be yet known of this celestial phenomenon:—• “I first observed the comet," observes Mr. Christie, “last night (Saturday) a minutes before 11 o'clock, and judge that it came to the meridian about 12. Its elevation above the horizon appeared about 10°, and the sun being at the time nearly below, its distance from the sun cannot much exceed 25°.

 

The night was remarkably light, and the moon uncovered by clouds—circumstances extremely unfavourable to the brilliancy of its appearance; and considering this, I should judge that, under more favourable circumstances, its splendour would be equal to that of any comet upon record—the head viewed with Capella (to the east of it) in brilliancy. The length of the tail, which, when the comet was on the meridian, pointed somewhat to the west of the zenith, extended about 15degrees;  and unlike the comet of 1811, it appeared to proceed immediately from the nucleus.

 

 I viewed it for some time through an excellent small reflector, by Watson, and observed, that the nucleus was much denser than that of the former comet, and that there was no separation between it and the coma, but that the body became gradually rarer, and in the upper part expanded into the tail; which appearance may arise from a very dense atmosphere surrounding the nucleus, and reaching to the rarer fluid forming the tail, if there be any distinction between the two fluids, as appears to have been the case with the comet 1811.

 

I may observe, that this as in all other comets, the appearance to the naked eye is much more striking and brilliant than through telescope. The Comet passed the meridian below the Pole, at the Royal Observatory, Greenwich, on Saturday, July 3, about midnight, when its place was determined as follows :

 

Apparent right ascension  6h. 51m. 56S

North polar distance, corrected for re fraction 43 d 18 m  47.s

 Mean time of observation .12h 6m 56s

 

 The Comet was again observed on Monday night (July 5), but not till it had passed the meridian, when the following observations was made :

Apparent right ascension . 7h. 0m 9s

 North Polar Distance 43 d 34m 48s

Mean time of observation  12h 36m 04s

 

This was comet 1819 also known as Trailes comet that was discovered on July 1st 1819 by the German astronomer Johann Georg Trailes. The comet was an easy naked eye object reaching between magnitude 1 to 2.



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Wednesday, 14 May 2025

A little ramble through Camelopardalis the Giraffe

 

We have another of the modern and dull constellations, quite possibly Camelopardalis the Giraffe is one of the dullest of the northern constellations. It was first created by the Dutch astronomer Petrus Plancius around 1613. There are some suggestions that originally the constellation represented a camel rather than a giraffe.

With Camelopardalis being a modern constellation there are no myths and legends associated with it.

Although the 18th largest constellation in the sky there are no bright stars and only alpha and beta might be glimpsed with the naked eye.



The brightest star is beta with a magnitude of 4.0 it is a G class supergiant and is cooler than the Sun, it lies around 870 light years away. It is a triple star system although you would need a telescope to see the two companion stars.

Beta is the brightest star in Camelopardalis at magnitude 4.0 Its a G1 supergiant 870 light years away.

Although alpha should be the brightest star using the Bayer system it isn’t with a magnitude of 4.2. As in the case with beta any sort of mist haze or moonlight would mean that both stars would be impossible to see with the naked eye.

However, alpha is interesting because it is one of the rare O class supergiant stars. Its surface temperature is a whopping 29,000 degrees compared with just 5,800 for our Sun. It lies at a massive 6,000 light years from Earth. I think we can safely say that at some point in the future this star is going to become a supernova and destroy itself in a massive explosion.

The only other star of interest here is the variable star Z Camelopardalis which is the prototype star for the Z Camelopardalis group of stars. It is known as a cataclysmic type variable star it is a dwarf nova, the mechanism behind the outbursts is different from classical nova. Dwarf Nova are fainter than the more classical nova. It varies in brightness between magnitude 9.8 to 14.5 meaning that a telescope is needed to observe it at all times.

The star was discovered in photographs taken in 1904 by Henry Park Hollis 1858-1939 a British astronomer who worked at the Royal Greenwich Observatory in London.

The only dep sky object I will refer you to is Kemble’s Cascade. It is an apparent line of more than 20 stars with brightnesses of between the 5th and 10th magnitude. It appears to flow into the open cluster NGC 1502.

Kemble’s Cascade is what is known as an asterism, a pattern of stars with a constellation. The group of stars we call the Plough is an asterism within the constellation of Ursa Major the Great Bear. The asterism was named by the astronomer Walter Scott Houston 1912-1993 who wrote The Deep Sky Wonders collum for the Sky and Telescope magazine from 1946-1993. He named it after a Franciscan friar and amateur astronomer Father Lucian Kemble 1922-1999 who wrote to Scott Houston and described it as a beautiful cascade of stars tumbling from the north west down to the open cluster NGC 1502. The stars are not part of the open cluster it is just a line-of-sight effect. It was after this letter in 1980 that Kemble’s Cascade was named.

I said at the beginning that this constellation was a faint constellation and broadly speaking Camelopardalis fills the large area of space between Capella in Auriga, Polaris the North Star and Cassiopeia. It has been said that if you come across an area of sky in the north with nothing in it, you have located the Giraffe!



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Tuesday, 13 May 2025

Asteroid Mancuria (Latin for Manchester) discovered in 1912

 On May 18th 1912 Harry Edwin Wood who was chief assistant at the Union Observatory in South Africa discovered an asteroid, it was named Mancuria after the city in which he was born, Manchester. He would discover 12 asteroids between 1911-1932. 

Mancuria is the Latin name for Manchester


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Monday, 12 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 mounting for Dollond telescope in 1865

 The Rev Frederick Howlett FRAS (1821-1908) purchased in 1865 a plain equatorial mounting from Thomas Cooke & Sons, it was made to carry either a 4 or 5 inch telescope. At the time that the mounting was ordered he was living at the St Augustine's Parsonage , Hurst Green , Sussex.

 Howlett used a 3 inch Dollond telescope, I am not sure when he purchased this telescope but it was before 1863. During the 1860s-1880s he used this small telescope to make extensive observations of sunspots.


                                                       www.therambling astronomer.co.uk

 

Sunday, 11 May 2025

A little ramble through 19th century astronomy - Remarkable Sunspots in 1871

                                                           

The accompanying sketch shows in a rough way the umbrae and a small portion of the penumbra of a sunspot that I observed on the 6th and 7th May 1871, and which was made remarkable by the presence of a reddish-brown object like a cloud, that seemed to hang over the nucleus of the principal umbra, apparently dividing it into two. Could this object be seen without the intervention of the dark glass, it would doubtless show a bright red instead of a reddish-brown colour; and from its fog like aspect, though it was well defined in outline and acuminated at both ends, the impression was inevitable that it hung at a certain altitude above the spot. 

                                                          Sunspot Drawing May 6/7 1871

However, it evidently had no motion distinct from the latter, as on the 7th May it occupied the same position as on the day before, but it was much reduced in size. On the 8th May it was seen no, longer, and the nucleus was now in one, seeming to show pretty clearly that its previous apparent division in two was really caused by the intervention of the brown cloud suspended over it, and that the phenomenon did not consist of two distinct nuclei with the brown object lying between them.

I am not aware that anything like this was observed before.

 J Birmingham , Millbrook, Tuam May 18th 1871


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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. 


                                                      www.theramblingastronomer.co.uk

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.


                                                     www.theramblingastronomer.co.uk



 

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.


www.theramblingastronomer.co.uk

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

Sunday, 4 May 2025

A Cooke telescope for the Brussels Observatory in 1880

 Yorkshire Gazette Saturday 15th May 1880 

Messrs T Cooke & Sons, opticians of this city, had the honour some time ago of receiving an order from the Belgium Government for an equatorial mounting for a telescope with an object glass of 15 inches diameter, which is to be placed in the Royal Observatory Brussels.

 The work has just been completed, and the instrument presents a fine specimen of mechanical art and skill. The tube about 21 feet in length, and the stand 13 feet high. The instrument is fitted with all the latest appliances, including clockwork of very delicate construction by which the telescope caused to follow the movement of the star on which it is fixed. The firm expect to pack and forward the instrument towards the end of the month.



                                                       www.theramblingastronomer.co.uk