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


                                                     www.theramblingastronomer.co.uk

 

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.



                                                     www.theramblinbgastronomer.co.uk

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


                                                         www.theramblingastronomer.co.uk


 

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

 

Saturday, 3 May 2025

Jupiter observed from Canada in 1896 with a Cooke telescope

 Dr J C Donaldson of Fergus, Ontario, Canada using a 3.5 inch Thomas Cooke telescope obtained a glimpse of the 9th magnitude star in Cancer just before it was occulted by Jupiter on May 22nd 1896. 

Several other observers had attempted to watch the occultation in Canada many with much larger telescopes but were unsuccessful.


                                                       www.theramblingastronomer.co.uk

Friday, 2 May 2025

A little ramble through Bootes the Herdsman

 The constellation of Bootes is sometimes associated with a herdsman who was placed in the sky for inventing the plough pulled by two oxen. It has also been associated as the driver of the wain, which is an old name for plough. However, he has also seen with the hunting dogs Asterion and Chara chasing the great bear around the sky. Asterion and Chara are the two old names for the hunting dogs connected with the constellation of Canes Venatici, although we still use the name Chara, Asterion has now become Cor Caroli. We will meet these two stars later when I look at Canes Venatici.

In another version of what the constellation represents is the idea that Bootes was seen as the shouting of the driver of the oxen or the shouting of the hunter to the dogs while chasing the bear.

There appears to be some confusion with Egyptian translations where Bootes sometimes gets confused in translation with Orion in this case they both can be seen as Horus. To Arabian astronomers like the Greek astronomers the constellation is seen as a herdsman.

The best way to pronounce Bootes is to think of the word co-ordinate.  Bootes is very prominent in the spring and early summer skies.  It is always a little bit difficult to work out the best shape to describe Bootes because it is a large constellation, and it is in a barren part of the sky.


The brightest star alpha or to give its proper name, Arcturus which  is also the brightest star in the northern hemisphere at magnitude 0. 0 and its name means the ‘Bear Keeper’.  In India it was regarded as Svati the Good Goer, while the Chinese called the star Ta Kio the Great Horn. Arcturus is an orange K0 class giant star 37 light years away. It is cooler but larger than the Sun.

One Arab name for Arcturus was Al Simak which means the leg of the lance bearer, while Al Biruni one of the great Arab astronomers called it the Second Calf of the Lion , the first being Spica the brightest star in Virgo.

Every star has its own story, but some are more curious than others. The bright orange star Arcturus, which can be found by following the curve of the handle of the Plough around and down, has an electrifying story with a twist involving the 1933 ‘Chicago Century of Progress Exposition’ in America.

Chicago had hosted its first big scientific fair in 1893. At the time it was believed that Arcturus was forty light years away, so when the second Exposition was planned for 1933, forty years after the first, it was decided to use the light from Arcturus to switch on the lights to the exhibition by hitting a photocell. A photocell is an electronic device that produces electricity when light falls upon it.

On May 27th, 1933, the light which left Arcturus in 1893, taking 40 years to reach earth, was channelled through a powerful telescope and directed on to a photocell to switch on the lights for the Exposition. Everything worked perfectly, except that today we know that Arcturus is only 37 light years away, not 40. The light had left the star not in 1893 but in 1896!

You might remember that I explained in the introduction to the constellations that the brightest 24 stars in each constellation have a Greek letter assigned to it with the brightest being alpha and the 24th or least bright one being omega. I also said that sometimes this does not follow and Bootes is another good example of this.

The second brightest star is epsilon which is the 5th letter of the Greek alphabet and has a magnitude of 2.4. Epsilon or Izar which means the ‘veil’. Izar is a K0 giant and is cooler than the Sun and is 203 light years away.

Eta or to give its Arab name Al Mufrid, the Solitary Star of the Lancer, a name which was given to the star  by the Arab astronomer  Ulug Beg, while another Arabic astronomer Al Kazwini calls it Al Rumh meaning the Lance of the Lance Bearer. Eta has a magnitude of 2.7 and is a G0 class start just a little hotter than the Sun and lies just 37 light years away.

Gamma is an A7 class star which is hotter than the Sun, it has a magnitude of 3.0 and is 87 light years away. Gamma is sometimes known as Seginus the meaning of which is unknown.  The Chinese refer to this star as Heuen Ko or heavenly spear.

The only other bright stars are Beta or Nekka meaning ‘Herdsman’ which can also refer to the whole constellation and is a magnitude 3.5 star and is 225 light years away. The Chinese called it Chaou Yaou which means to beckon or move. Nekka is a G8 giant slightly cooler than the Sun.

I will mention one deep sky object which is NGC 5466 a globular cluster. The NGC stands for New General Catalogue this was introduced in 1888, although not new today we still use the term. This globular cluster is approximately 51,800 light years from Earth. The cluster was first discovered by the British astronomer William Herschel in 1784. Herschel had discovered the planet Uranus in 1781. At magnitude 9.2 you would need a telescope to be able to see NGC 5466. This cluster lies about 52,800 light years from the Galactic centre.

There is one important meteor shower that can be seen coming from the constellation of Bootes. This is the Quadrantids and is usually seen around the 4th of January. There can be between 60-100 meteors per hour seen in the sky, however with this shower the peak of activity will only last for a few hours rather than the whole night.

If you look up into the sky on any clear night you will be unlucky not to see at least one meteor or shooting star as some people like to call them. These meteors have nothing at all to do with stars. They are the tiny grains of dust that are left behind by a comet or an asteroid as it travels around the Sun. If the Earth happens to cut across the path of one of those trails of dust left by comets we see lots of meteors in the sky. This is called a meteor shower, there are several prominent ones each year. We see the meteors when they burn up as they enter the atmosphere of the Earth and for just a moment, we see a streak of light dash across the sky.

 The Quadrantids are associated not with a comet, but an asteroid called 2003 EH1.

The Quadrantids take their name from the now defunct constellation of Quadrans Muralis the Mural Quadrant, this was an instrument attached to a wall that would allow astronomers to measure the positions of stars in the sky. It could measure up to 90 degrees or one quarter of the sky. The constellation can no longer be seen on modern star maps.  It was created by the French astronomer Jérôme Lalande 1732-1808 in 1795. It was located between the constellations of Boötes and Draco, near the tail of Ursa Major or Great Bear.

The constellation had ceased to be used by astronomers towards the end of the 19th century.  The Mural Quadrant is the only defunct constellation referred to by astronomers today, albeit thought the Quadrantid meteor shower.

Don’t forget if you see a meteor, you must make a wish!!


                                                    www.theramblimngastronomer.co.uk