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Astronomical Information for Taunton during September 2021

Starfish imageIntroduction

Welcome to – Astronomical Information from the UK Hydrographic Office

This page provides some astronomical information on a monthly basis for those of you living in the Taunton area. Timings are in BST (British Summer Time) unless otherwise noted. Latest additions or updates are highlighted with a red border.

This month we have sections on:


2021 Astronomical and Calendarial Sheet

Download Adobe Acrobat Reader Additional information on the phases of the Moon, the seasons, summer times, eclipses, chronological cycles and eras, religious calendars, the civil calendar and holiday dates in the United Kingdom can be found in HMNAO's Astronomical and Calendarial Sheet No. 108 for 2021. This is a pdf document for which a document reader can be downloaded by clicking on the Adobe Reader icon above.

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This web page can also be accessed from outside the UK Hydrographic Office on

↻ The last update to this page was made on Monday, 2021 September 20 at 10:36:25 BST.

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Starfish imageSolstices & Equinoxes

Solstices and Equinoxes diagram courtesy NASA (357x432) The Autumnal Equinox for the northern hemisphere (or the Vernal Equinox for the southern hemisphere) takes place on Wednesday September 22nd at 19:21 GMT or 20:21 BST.

On this day, the Sun crosses the celestial equator moving southwards and the approximate length of night and day are the same. The word 'equinox' is derived from the Latin words 'aequus' meaning equal and 'nox' meaning night. The number of daylight hours will continue to decrease until we reach the minimum amount of daylight at the northern hemisphere Winter Solstice on Tuesday December 21st at 15:59 GMT. Please click on the image above to see a larger version of the diagram demonstrating the occurrence of solstices and equinoxes.

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Starfish imageThe Sun

  animation of Solar Dynamics Observatory images of the Sun courtesy of NASA An animated view of the Sun's disk over the last twenty eight days is shown in the image on the left. North is at the top of the image and east is to the left. These images come from the Helioseismic and Magnetic Imager instrument on the NASA Solar Dynamics Observatory (SDO) satellite. More multi-wavelength data from the SDO can be found here.

After a spotless run of only three days, an active region designated AR2871 is situated very close to the south-eastern limb of the Sun. It is actually the old feature AR2860, returning after a two-week transit around the farside of the Sun. This potent feature produced one M-class solar flare and twenty one C-class solar flares during late August. A very dynamic prominence composed of unstable magnetic fields some 300,000 km wide is also hovering above this active region. A second active region may be forming in the north-eastern quadrant of the Sun not too far from the equatorial limb. The total number of spotless days for 2021 remains at fifty nine, or 22% of the year so far. Solar winds are currently blowing with velocities of up to 320 km/s and the planetary Kp geomagnetic activity index is likely to peak at 1 (quiet) today. There is a modestly-sized coronal hole in the south-eastern quadrant close to the central meridian of the Sun. Solar winds emanating from this feature could reach the Earth on September 23rd–24th. The overall amount of solar activity remains at very low levels.

NASA reported that a reversal of the Sun's magnetic field took place at the start of 2014 indicating that the maximum of Solar Cycle 24 had been reached. A plot of sunspot numbers, both observed and predicted versus time indicates that the solar maximum of Solar Cycle 24 was more complex than had been previously predicted. The maximum was double-peaked in a similar manner to that of the previous maximum of 2001/2002. The individual peaks occurred in 2011 and 2014 with the latter being the larger of the two. However, sunspot numbers were significantly down on the predictions made for the maximum — indeed Solar Cycle 24 may be the weakest in the last 100 years or so i.e. since Solar Cycle 14.

The declining phase of the solar cycle brings increased numbers of cosmic rays to the Earth, an increased frequency of 'pink' aurorae and a slight dimming of the Sun of approximately 0.1% in terms of the total solar irradiance. TSIS-1 was launched on December 15th 2017, which will monitor the Sun over a five-year period covering the whole of the current solar minimum. Cooling and contraction of the Earth's upper atmosphere in response to the changes on the Sun due to the solar minimum also delayed the orbital decay of satellites such as the Chinese space station, Tiangong 1, which returned to Earth on Monday April 2nd 2018 at 00:16 UTC. The Sun's magnetic field and solar winds provide some protection for the Earth from cosmic rays. A recent paper in the journal Space Weather claims that this solar minimum could see a rise in the number of cosmic rays reaching the Earth by as much as 30% due to the weakening magnetic field of the Sun and reduced levels of solar winds. This could mean an increased risk of radiation exposure for travellers on commercial airlines and possible changes to the climate.

During the post maximum phase of the solar cycle individual energetic events can spawn some of the most powerful flares and coronal mass ejections of the cycle. The so-called Carrington event on September 1st–2nd 1859 during Solar Cycle 10 is a good example of just what might ensue from this type of violent outburst. On 2020 September 15th NASA and NOAA announced that a minimum of the Sun's activity had been reached in December 2019 bringing to an end the old Solar Cycle 24. Predictions are that the new Solar Cycle 25 will be a weak one, similar to its predecessor, peaking in 2025. It is likely to be a deep minimum with long periods without much sunspot or flare activity. Space weather will be dominated by solar winds and cosmic rays rather than sunspots and solar flare activity.

The latest information on solar activity can be found at and at the Space Weather Prediction Center Space Weather Enthusiasts Dashboard.

If an auroral display is possible or likely, warnings can be received from AuroraWatch UK. More UK-focused geomagnetic data can be found at the British Geological Survey web site.

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Starfish imageThe Moon

The sequence of Moon phases for this month and their designations are shown in the following animation:

Continuous Moon Phase animation
  Moon phases for September 2021 are as follows:
New Moon symbol New Moon Tuesday September 7th at 01:52 BST
Lunation 1221
First Quarter symbol First Quarter Monday September 13th at 21:39 BST
Full Moon symbol Full Moon Tuesday September 21st at 00:55 BST
'Harvest Moon'
Last Quarter symbol Last Quarter Wednesday September 29th at 02:57 BST

The Moon is at perigee (i.e. nearest to the Earth) on Saturday September 11th at 11:03 BST when it is 368,461 km from the Earth. It is at apogee (i.e. furthest from the Earth) on Sunday September 26th at 22:44 BST when it is 404,640 km from the Earth.

There are no occultations of either planets or bright stars this month. The next planetary occultations for Mercury and Venus will take place in early November.

Please follow the New Moon link above to find out more about our Crescent Moon Watch program which involves making a sighting of the new crescent moon as early as possible after the instant of New Moon each month.

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Starfish imageEclipses

Partial eclipse of the Sun There are four eclipses visible from the Earth during 2021 — two lunar eclipses, one total and one partial and two solar eclipses, one annular and one total. Parts of two of the eclipses are visible from the United Kingdom, namely the partial phase of the annular eclipse of the Sun and some of the partial eclipse of the Moon. The total eclipses of the Sun and Moon are not visible from the United Kingdom.

A total eclipse of the Moon occurred on Wednesday May 26th 2021. It was visible in its entirety from south-westernmost Alaska, the Aleutian Islands, the Hawaiian Islands, Polynesia, the central Pacific Ocean region, New Zealand, Melanesia, Micronesia, central and eastern Australia and parts of Antarctica. Parts of the eclipse were visible from the Americas except north-eastern Canada and eastern parts of South America, Indonesia, the Philippines, Japan, eastern Asia, north-easternmost Russia and the eastern half of the Indian Ocean. The eclipse began at 08:46 UT and ended at 13:51 UT. The Moon entered the umbral shadow at 09:45 UT. Totality began at 11:10 UT and ended at 11:28 UT. The Moon left the umbral shadow at 12:53 UT. The eclipse was not visible from the United Kingdom.

An annular eclipse of the Sun occurred on Thursday June 10th 2021. It was visible as a partial eclipse from the north-eastern part of North America, the Arctic Ocean, most of Greenland, Iceland, northern Europe (including the British Isles), Scandinavia, most of Russia, Mongolia and most of China. The path of annularity began over central Ontario and crossed over north-western Quebec, the southern part of Baffin Island, the north-western part of Greenland, the North Pole (for the only time this century) and the north-eastern part of Siberia. The eclipse began at 08:12 UT and ended at 13:11 UT. The annular phase started at 09:50 UT and ended at 11:33 UT. The maximum duration of annularity of 3m 48s took place at 10:42 UT over the sea between Ellesmere Island and north-western Greenland. From Taunton, the partial eclipse started at 10:04 BST and ended at 12:18 BST. The maximum obscuration occurred high in the south-eastern sky at 11:08 BST when 21.4% of the Sun was obscured.

A deep partial eclipse of the Moon occurs on Friday November 19th 2021. It is visible in its entirety from most of North America except the easternmost parts, Mexico, the eastern and central Pacific Ocean regions and north-eastern parts of Russia. Parts of the eclipse are visible from Scandinavia, the British Isles, Iceland, South and Central America, Australasia, Japan, the Philippines, most of Indonesia, eastern and northern Asia. The eclipse starts at 06:00 UT and ends at 12:06 UT. The umbral phase of the eclipse starts at 07:18 UT and ends at 10:47 UT. The maximum of the eclipse occurs at 09:03 UT with a magnitude of 0.978. The eclipse is visible in part from the United Kingdom. From Taunton, the partial eclipse starts at 06:00 UT and ends at 07:35 UT at moonset.

A total eclipse of the Sun occurs on Saturday December 4th 2021. It is visible as a partial eclipse from Antarctica, the South Atlantic Ocean, the southernmost part of South Africa, the South Indian Ocean, Tasmania and the southernmost part of Australia. The path of totality starts approximately 450 km to the east of the Falkland Islands, crosses the Weddell Sea and the Ronne Ice Shelf, Ellsworth Land and ends over the Amundsen Sea, approximately 500 km from the coast of western Antarctica. The eclipse starts at 05:29 UT and ends at 09:38 UT. The total phase of the eclipse starts at 07:00 UT and ends at 08:07 UT. The maximum duration of totality is 1m 57s at 07:33 UT over the Ronne Ice Shelf in western Antarctica. The eclipse is not visible from the United Kingdom.

Further information on all the eclipses in 2021 can be found on the Eclipses Online web pages. This web site provides information on both solar and lunar eclipses in the period from 1501 CE to 2100 CE. Global circumstances of both solar and lunar eclipses are provided as well as local circumstances of the solar eclipses based on a gazetteer of approximately 1500 locations worldwide. Eclipses for next year, 2022, are also available.

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Starfish imageThe Planets

Planets visible with the naked eye ...

Mercury image

Mercury remains in its best evening apparition of the year for southern hemisphere observers. However, for northern observers, it is the worst apparition of the year with Mercury setting very shortly after the Sun. It reaches greatest eastern elongation on Tuesday September 14th. Mercury is very low in the west south-western evening twilight sky, fading from magnitude +0.0 at the start of the month to magnitude +1.5 at the end of September. It lies 7° south of the waxing crescent moon on Wednesday September 8th, 1.7° south of Spica (α Virginis) on Thursday September 23rd and 1.7° south of Spica again on Thursday September 30th.

Venus image

Venus lies in the west south-western evening twilight sky at an elongation which increases from 40° to 45° as the month progresses. Despite the increase in elongation, it remains poorly placed for northern observers due to the unfavourable angle of the ecliptic. It brightens somewhat from magnitude −4.0 at the start of the month to −4.2 at the end of September. Venus lies 1.7° north of Spica (α Virginis) on Sunday September 5th and 4° south of the waxing crescent moon on Friday September 10th.

Mars image

Mars is now too close to the Sun to be observed and reaches conjunction with the Sun on Friday October 8th. It will re-emerge into the morning twilight in the constellation of Libra at the end of November.

Jupiter image

Jupiter rises around an hour before sunset and sets one to four hours before sunrise. It lies in the constellation of Capricornus throughout September. Jupiter continues its retrograde or westward motion during September and fades slightly from magnitude −2.8 at the start of the month to magnitude −2.7 at the end of September. It lies 4° north of the waxing gibbous moon on Saturday September 18th.

Saturn image

Saturn rises one to two hours before sunset and sets two to four after midnight. It lies in the western part of the constellation of Capricornus throughout September. Saturn continues its retrograde or westward motion during September and fades somewhat from magnitude +0.3 at the start of the month to magnitude +0.5 at the end of September. It lies 4° north of the waxing gibbous moon on Friday September 17th. The north side of the ring plane is exposed with a tilt of 18° with the ring system spanning nearly 43 arcseconds while the planet's disk is only 18 arcseconds wide.

Planets visible with Binoculars ...

Uranus image

Uranus is visible reasonably high in the southern sky before the start of morning twilight throughout September, rising in the mid-evening. It is a blue-green object which remains at magnitude +5.7 throughout September. Uranus lies in the central southern part of the constellation of Aries where it remains for the rest of the year. It lies approximately 5.5° north of the fourth magnitude A9 giant star 87 Ceti (μ Ceti). This planet can also be glimpsed with the naked eye under optimum conditions.

Neptune image

Neptune is visible in the southern sky just after midnight throughout September, rising around sunset. Neptune is a bluish object which remains at magnitude +7.8 throughout September. It lies in the north-eastern part of the constellation of Aquarius where it remains for the remainder of the year. Neptune lies approximately 9.8° to the north east of the third magnitude M2.5 red-giant star Hydor (λ Aquarii). It is normally visible with good binoculars under optimum conditions although it can also be difficult to distinguish Neptune from other stellar objects of a similar magnitude.

... & Telescopes!

Pluto image

Pluto rises an hour or so before sunset and sets before morning twilight, making it visible in the southern sky around midnight throughout September for observers using larger telescopes. It lies in the north-eastern part of the constellation of Sagittarius about 11.8° to the south west of the third magnitude binary pair known as Dabih Major and Dabih Minor (β Capricorni) in mid-September. Strictly speaking, this is a dwarf planet which was demoted from the ranks of the 'bona-fide' planets at the 2006 International Astronomical Union General Assembly in Prague. At magnitude +14.7, you will need a much larger telescope to find this remote member of the Solar System.

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Starfish imageZodiacal Light

Zodiacal Light The rarely-spotted Zodiacal Light is best seen in the half hour or so before astronomical twilight starts in the morning or in the half hour or so after astronomical twilight ends in the evening. It is best seen when the ecliptic, the path the Sun takes in the night sky, is at a steep angle to the horizon. In northerly latitudes, this occurs in the western evening post-twilight sky in February and March and the eastern morning pre-twilight sky in September and October. The Zodiacal Light appears as a large, softly radiant pyramid of light with its base near the horizon and its axis centred on the Zodiacal constellations. It appears to be about as bright as the Milky Way, consequently a dark, unpolluted sky without haze is essential to see this phenomenon. Beware, it can easily be confused with the twilight itself. In the photograph, the Zodiacal Light is on the left and the Milky Way is on the right. For Taunton, astronomical twilight starts in the morning at around 04:20 BST at the beginning of the month and at 05:20 BST at the end of the month. The cause of this so-called 'false dawn' is sunlight reflecting of a lens-shaped cloud of dust in the plane of the inner solar system.

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Starfish imageMeteor Showers

Perseid meteors in 2010 There are no significant meteor showers active during September. The next shower exhibiting moderate numbers of fast meteors with long trains is the Orionids at the end of the third week of October. Further information on this and other meteor showers occurring during 2021 can be found at the International Meteor Organization and their 2021 Meteor Shower Calendar.

It is worth noting that bright sporadic meteors and fireballs are possible at any time e.g. the fireball observed over many parts of England and Scotland on Saturday March 3rd 2012 at 21:40 GMT. Larger events, known as bolides, are rarer. Typically, this is a very bright fireball reaching an apparent magnitude of −14 or so, perhaps three times as bright as a full moon. Even rarer are the superbolides, events with apparent magnitudes of −17 or so, around 50 times brighter than the full moon. A recent example of a superbolide was the Chelyabinsk meteor of Friday 15th February 2013 at 03:20 UTC which may have been a 20-metre diameter near-Earth asteroid.

A fireball was seen over a significant fraction of the United Kingdom and northern Europe on Sunday February 28th at 21:54 UT lasting approximately 3.5 seconds. It was estimated to be a magnitude −9 fireball which generated a sonic boom as it fell. Fragments of the object may have impacted the Earth in the area north of Cheltenham in Gloucestershire. Its solar-system point of origin may lie in the asteroid belt between Mars and Jupiter. It has since been reported that at least part of the carbonaceous chondrite fell at a property in Winchcombe in Gloucestershire making it the first UK-based meteorite find in the past 30 years. The significance of this type of dark stony meteorite lies in the fact that its chemistry is similar to that of the early Solar System.

A loud sonic boom was heard at 14:58 UT on Saturday March 20th 2021. It rattled windows and shook homes for about 20 to 30 seconds and was heard over large tracts of Dorset, Devon, Somerset and Jersey. An explosion, an earthquake, thunder and a sonic boom from an RAF aircraft have all been ruled out. The culprit appears to be a daylight fireball or bolide which may have landed in the Bristol Channel. It has been photographed and may also have been detected on a Eumetsat weather satellite image. To be visible in daylight, the meteor must have been of a significant size, large enough for debris to have reached the ground. Its track through the atmosphere may be revealed by analysis of photographic material.

Another loosely-related phenomenon is the re-entry of space debris from space vehicles and satellites whose orbits are decaying to the point where they burn up in the Earth's atmosphere. A couple of well-reported examples of this occurred at around 23:00 BST on Friday September 21st 2012 as well as the return of the GOCE satellite just after midnight on Tuesday November 12th 2013.

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Starfish imageComets

Comet McNaught - January 2007There are a number of comets around the sky at the moment. However, most of them require telescopic assistance to see them and some may be too far south in the sky to be seen by observers based in the United Kingdom. Here is a brief summary of the comets brighter than 11th magnitude that may be accessible to observers with binoculars or small telescopes in the northern hemisphere.

C/2019 L3 (Atlas) is currently a tenth magnitude object in the constellation of Lynx. It remains in Lynx for the first half of the month and then spends the remainder of September in Auriga. It should brighten slowly by about 0.3 magnitudes as the month progresses and will be visible with small telescope reasonably high in the eastern morning twilight sky in the easternmost part of Auriga. It will reach perihelion on January 9th 2022.

One possibility for a naked-eye comet in the run up to Christmas is C/2021 A1 (Leonard) in early/mid-December. At the moment, this comet is an obscure fourteenth magnitude object in Ursa Major which will brighten more than a magnitude during September. If it reaches naked-eye visibility, it could be visible low in the west north-western sky after sunset in the constellation of Böotes at the end of the first week of December. As it is heading towards perihelion in early January 2022, it will be getting lower in the sky as it moves towards the Sun.

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Starfish imageInternational Space Station

NASA International Space Station photo If you want to look for the International Space Station (ISS) as it passes over Taunton, please have a look at the predictions page on the Heavens Above web site. The ISS is at least as bright as a first magnitude star and can approach the brightness of Venus under favourable conditions. Similarly, if you want to look for the core module of the new, third generation Chinese space station, Tianhe-1, predictions for this 'under-construction' space station can be found on this page. This module, the first of three parts, was launched on Thursday April 29th 2021. Tianhe-1 is significantly fainter than the ISS, normally about as bright as a third of fourth magnitude star. Predictions for other satellites may also be obtained from the Heavens Above web site.

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Starfish imageAurorae

Ovation auroral prediction for the northern hemisphere The above image is a 30 minute forecast of the location and probability of auroral activity based loosely on a model developed at Johns Hopkins' Applied Physics Laboratory known as the Ovation Aurora Forecast model. It provides estimates of the energy per unit area on the Earth's atmosphere from observations of the solar wind and interplanetary magnetic field made by the Advanced Composition Explorer satellite in conjunction with empirical relationships derived from the Defense Meteorological Satellite Program. It shows where the aurora is most likely to be seen and how bright it might be. The model generates a global estimate of power, called the Hemispheric Power, deposited into the atmosphere in gigawatts (GW). For powers of less than 20GW, little or no aurora may be visible. For powers of 20-50 GW, you may need to be relatively close to the aurora to see it. For values above 50 GW, the aurora should be easily observable, active and mobile. For values above 100 GW, this is considered to be a significant storm where the aurora may be visible from hundreds of miles away. The current prediction is downloaded when you load this page. If you want to download the latest model, simply reload this page or press F5. If you want to see the full-sized map, please click on the above image.

If an auroral display is possible or likely, warnings can be received from AuroraWatch UK. More UK-focused geomagnetic data can be found at the British Geological Survey web site.

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Starfish imageSky chart for mid-September at 22:00 BST for Taunton

Sky chart for mid-September 2021 from Taunton at 22:00 BST The above sky chart, generated from the web site, shows what the night sky looks like at 22:00 BST on Wednesday September 15th 2021 from Taunton. The night sky will look the same an hour later at 23:00 BST at the beginning of the month and an hour earlier at 21:00 BST at the end of the month. Please click on the chart to see a full-sized sky chart image. If you want to generate your own star chart for Taunton for another date and/or time, please follow this link.

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Starfish imageRise/set times (BST) for the Sun & Moon for Taunton

In September 2021, the amount of daylight (measured from sunrise to sunset) decreases from 13 hours 32 minutes at the start of the month to 11 hours 41 minutes at the end of the month. Total daylight (sunrise to sunset) for the month is 378 hours 14 minutes.

start and end times of civil, nautical and astronomical twilights.

September 2021
Date &
Rise/Set timesDay
h mh mh mh mh m
01Wed06:2619:58** **17:1813:32
15Wed06:4819:2617:15** **12:38
30Thu07:1118:52** **16:4611:41
** ** No phenomenon on that day
PLEASE NOTE: These times are in Greenwich Mean Time (GMT) except between 01:00 GMT on March 28th and 01:00 GMT on October 31st when the times are in BST (British Summer Time) which is one hour in advance of GMT.

Useful area for table of rise/set times The timings in the table above should be accurate to within 1–2 minutes inside the red circle superimposed on the map shown on the left.

Rising and setting times for the Sun, Moon and planets and times of twilights for other locations can be obtained from HMNAO's Websurf web pages using the Rise, Set and Twilight Times option.

The actual times at which the Sun will just appear, or disappear, will depend on the difference between the altitudes of the observer and the local horizon and the actual refraction, which depends on the meteorological conditions along the light path. Differences of a minute or so from the tabulated times are to be expected.

For the drivers amongst you, the 'Hours of Darkness', as defined in the Road Vehicle Lighting Regulations (1989), start half an hour after sunset and end half an hour before the following sunrise. Headlights should be used during the Hours of Darkness and sidelights in the half hour periods after sunset and before sunrise. These timings can also be obtained from HMNAO's Websurf web pages using the Rise, Set and Twilight Times option.

For the pilots amongst you, night, according to Statutory Instrument 2016 No. 765, The Air Navigation Order 2016, Schedule I (Interpretation), Article 2, means 'the time from half an hour after sunset until half an hour before sunrise (both times inclusive), sunset and sunrise being determined at surface level'. In other words, the night time period starts at the beginning of the Hours of Darkness and finishes at the end of the Hours of Darkness. In the United States, the Federal Aviation Administration (Federal Aviation Regulations, Section 1.1) defines night as the time between the end of evening civil twilight and the beginning of morning civil twilight as published in the American Air Almanac, converted to local time. Sunset to the following sunrise can also be defined as night in the United States as well as one hour after sunset to one hour before sunrise. By the way, flying in a total eclipse of the Sun does not count as night flying!

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Last modified: Monday, 20 September 2021 at 10:36:25 BST