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Warthog in a eating position.
They frequently get down like this when eating and will also "walk" like this sa they continue to eat.They are very spooky and will run at the blink of an eye.
Off beanbag. 20D W/100-400mm lens.
5 Jan 2025, 03:33 UT; Spotsylvania, Virginia USA. Bortle 4.5 zone.
Celestron C8 SCT at f/10.1. Orion Atlas AZ/EQ-G mount. Mallincam DS26cTEC camera, bin 1x1, exposure 16s, single frame, Optolong L'eNhance filter, no guiding, no calibration frames, sensor -5°C. Captured in Sharpcap Pro. Processed in PixInsight and Photoshop.
IDENTIFICATION OF Rigel BC
In the absence of a plate-solved location for Rigel BC the following information was considered:
1. Positive -- Published position angle (202° East of North) is consistent with labelled BC. Per ASTAP this image does not have standard orientation, e.g. it does not show North in the standard position -- up (0°). A corrected image would be rotated 7° and flipped on the horizontal axis for standard alignment with North, which puts the labelled star near the correct position.
2. Negative -- The brightest star in the field (besides Rigel A) is magnitude 6.35 and the nearby dimmer stars are approx. magnitude 10. The image of the labelled star BC (magnitude 7.5) is between them in size (brightness) but appears closer to magnitude 10 than 6.
3. Negative -- The separation of A from labelled BC in the image is roughly estimated from the image at 1 arcmin, not the expected 0.16 arcmin (9.5 arcsec).
4. Positive -- It is consistent with other posted amateur images of Rigel A & B.
BOTTOM LINE
I have 80% confidence that Rigel BC is correctly identified in this image, but another star could be obscured in the asymmetrical flare. An occulting bar may be used to verify dim Rigel BC against its brilliant companion in a subsequent image.
Appearance: Bright light blue star (Rigel A) and dim companions (Rigel B, C, and D), with adjacent variable star λ Eri (magnitude 6.35) at 3:00 position. The severe halo/flare around Rigel may be due to the filter, and may be asymmetrical due to moderate sensor tilt in the system.
Clouds: clear
Transparency: average
Seeing: below average
Apparent Magnitude (USNO): A 0.5-0.18, BC 7.5-7.6
Separation A-BC: 9.5 arcsec
Image scale:
Moon age, illuminated: xx, xx
Azimuth: xx°
Altitude: xx°
from Wikipedia
Rigel is a blue supergiant star in the constellation of Orion. It has the Bayer designation β Orionis, which is Latinized to Beta Orionis and abbreviated Beta Ori or β Ori. Rigel is the brightest and most massive component – and the eponym – of a star system of at least four stars that appear as a single blue-white point of light to the naked eye. This system is located at a distance of approximately 860 light-years (260 pc) from the Sun.
A star of spectral type B8Ia, Rigel is 120,000 times as luminous as the Sun, and is 18 to 24 times as massive, depending on the method and assumptions used. Its radius is more than seventy times that of the Sun, and its surface temperature is 12,100 K. Due to its stellar wind, Rigel's mass-loss is estimated to be ten million times that of the Sun. With an estimated age of seven to nine million years, Rigel has exhausted its core hydrogen fuel, expanded, and cooled to become a supergiant. It is expected to end its life as a type II supernova, leaving a neutron star or a black hole as a final remnant, depending on the initial mass of the star.
Rigel varies slightly in brightness, its apparent magnitude ranging from 0.05 to 0.18. It is classified as an Alpha Cygni variable due to the amplitude and periodicity of its brightness variation, as well as its spectral type. Its intrinsic variability is caused by pulsations in its unstable atmosphere. Rigel is generally the seventh-brightest star in the night sky and the brightest star in Orion, though it is occasionally outshone by Betelgeuse, which varies over a larger range.
A triple-star system is separated from Rigel by an angle of 9.5 arc seconds. It has an apparent magnitude of 6.7, making it 1/400th as bright as Rigel. Two stars in the system can be seen by large telescopes, and the brighter of the two is a spectroscopic binary. These three stars are all blue-white main-sequence stars, each three to four times as massive as the Sun. Rigel and the triple system orbit a common center of gravity with a period estimated to be 24,000 years. The inner stars of the triple system orbit each other every 10 days, and the outer star orbits the inner pair every 63 years. A much fainter star, separated from Rigel and the others by nearly an arc minute, may be part of the same star system.
In 2016, the International Astronomical Union (IAU) included the name "Rigel" in the IAU Catalog of Star Names. According to the IAU, this proper name applies only to the primary component A of the Rigel system. The system is listed variously in historical astronomical catalogs as H II 33, Σ 668, β 555, or ADS 3823. For simplicity, Rigel's companions are referred to as Rigel B, C, and D; the IAU describes such names as "useful nicknames" that are "unofficial". In modern comprehensive catalogs, the whole multiple star system is known as WDS 05145-0812 or CCDM 05145–0812.
The designation of Rigel as β Orionis (Latinized to beta Orionis) was made by Johann Bayer in 1603. The "beta" designation is usually given to the second-brightest star in each constellation, but Rigel is almost always brighter than α Orionis (Betelgeuse). Astronomer J.B. Kaler speculated that Bayer assigned letters during a rare period when variable star Betelgeuse temporarily outshone Rigel, resulting in Betelgeuse being designated "alpha" and Rigel designated "beta". However, closer examination of Bayer's method shows that he did not strictly order the stars by brightness, but instead grouped them first by magnitude, then by declination. Rigel and Betelgeuse were both classed as first magnitude, and in Orion the stars of each class appear to have been ordered north to south.
Rigel has many other stellar designations taken from various catalogs, including the Flamsteed 19 Orionis (19 Ori), the Bright Star Catalogue entry HR 1713, and the Henry Draper Catalogue number HD 34085. These designations frequently appear in the scientific literature,[ but rarely in popular writing. Rigel is listed in the General Catalogue of Variable Stars, but since its familiar Bayer designation is used instead of creating a separate variable star designation.
Rigel is an intrinsic variable star with an apparent magnitude ranging from 0.05 to 0.18. It is typically the seventh-brightest star in the celestial sphere, excluding the Sun, although occasionally fainter than Betelgeuse. Rigel appears slightly blue-white and has a B-V color index of −0.06. It contrasts strongly with reddish Betelgeuse.
Culminating every year at midnight on 12 December, and at 9:00 pm on 24 January, Rigel is visible on winter evenings in the Northern Hemisphere and on summer evenings in the Southern Hemisphere. In the Southern Hemisphere, Rigel is the first bright star of Orion visible as the constellation rises. Correspondingly, it is also the first star of Orion to set in most of the Northern Hemisphere. The star is a vertex of the "Winter Hexagon", an asterism that includes Aldebaran, Capella, Pollux, Procyon, and Sirius. Rigel is a prominent equatorial navigation star, being easily located and readily visible in all the world's oceans (the exception is the area north of the 82nd parallel north).
Rigel's spectral type is a defining point of the classification sequence for supergiants.[36][37] The overall spectrum is typical for a late B class star, with strong absorption lines of the hydrogen Balmer series as well as neutral helium lines and some of heavier elements such as oxygen, calcium, and magnesium.[38] The luminosity class for B8 stars is estimated from the strength and narrowness of the hydrogen spectral lines, and Rigel is assigned to the bright supergiant class Ia.[39] Variations in the spectrum have resulted in the assignment of different classes to Rigel, such as B8 Ia, B8 Iab, and B8 Iae.
As early as 1888, the heliocentric radial velocity of Rigel, as estimated from the Doppler shifts of its spectral lines, was seen to vary. This was confirmed and interpreted at the time as being due to a spectroscopic companion with a period of about 22 days. The radial velocity has since been measured to vary by about 10 km/s around a mean of 21.5 km/s.
In 1933, the Hα line in Rigel's spectrum was seen to be unusually weak and shifted 0.1 nm towards shorter wavelengths, while there was a narrow emission spike about 1.5 nm to the long wavelength side of the main absorption line. This is now known as a P Cygni profile after a star that shows this feature strongly in its spectrum. It is associated with mass loss where there is simultaneously emission from a dense wind close to the star and absorption from circumstellar material expanding away from the star.
The unusual Hα line profile is observed to vary unpredictably. It is a normal absorption line around a third of the time. About a quarter of the time, it is a double-peaked line, that is, an absorption line with an emission core or an emission line with an absorption core. About a quarter of the time it has a P Cygni profile; most of the rest of the time, the line has an inverse P Cygni profile, where the emission component is on the short wavelength side of the line. Rarely, there is a pure emission Hα line. The line profile changes are interpreted as variations in the quantity and velocity of material being expelled from the star. Occasional very high-velocity outflows have been inferred, and, more rarely, infalling material. The overall picture is one of large looping structures arising from the photosphere and driven by magnetic fields.
Rigel has been known to vary in brightness since at least 1930. The small amplitude of Rigel's brightness variation requires photoelectric or CCD photometry to be reliably detected. This brightness variation has no obvious period. Observations over 18 nights in 1984 showed variations at red, blue, and yellow wavelengths of up to 0.13 magnitudes on timescales of a few hours to several days, but again no clear period. Rigel's color index varies slightly, but this is not significantly correlated with its brightness variations.
From analysis of Hipparcos satellite photometry, Rigel is identified as belonging to the Alpha Cygni class of variable stars, defined as "non-radially pulsating supergiants of the Bep–AepIa spectral types". In those spectral types, the 'e' indicates that it displays emission lines in its spectrum, while the 'p' means it has an unspecified spectral peculiarity. Alpha Cygni type variables are generally considered to be irregular or have quasi-periods. Rigel was added to the General Catalogue of Variable Stars in the 74th name-list of variable stars on the basis of the Hipparcos photometry, which showed variations with a photographic amplitude of 0.039 magnitudes and a possible period of 2.075 days. Rigel was observed with the Canadian MOST satellite for nearly 28 days in 2009. Milli-magnitude variations were observed, and gradual changes in flux suggest the presence of long-period pulsation modes.
From observations of the variable Hα spectral line, Rigel's mass-loss rate due to stellar wind is estimated be (1.5±0.4)×10−7 solar masses per year (M☉/yr)—about ten million times more than the mass-loss rate from the Sun.[52] More detailed optical and K band infrared spectroscopic observations, together with VLTI interferometry, were taken from 2006 to 2010. Analysis of the Hα and Hγ line profiles, and measurement of the regions producing the lines, show that Rigel's stellar wind varies greatly in structure and strength. Loop and arm structures were also detected within the wind. Calculations of mass loss from the Hγ line give (9.4±0.9)×10−7 M☉/yr in 2006-7 and (7.6±1.1)×10−7 M☉/yr in 2009–10. Calculations using the Hα line give lower results, around 1.5×10−7 M☉/yr. The terminal wind velocity is 300 km/s. It is estimated that Rigel has lost about three solar masses (M☉) since beginning life as a star of 24±3 M☉ seven to nine million years ago.
Rigel's distance from the Sun is somewhat uncertain, different estimates being obtained by different methods. Old estimates placed it 166 parsecs (or 541 light years) away from the Sun. The 2007 Hipparcos new reduction of Rigel's parallax is 3.78±0.34 mas, giving a distance of 863 light-years (265 parsecs) with a margin of error of about 9%. Rigel B, usually considered to be physically associated with Rigel and at the same distance, has a Gaia Data Release 3 parallax of 3.2352±0.0553 mas, suggesting a distance around 1,000 light-years (310 parsecs). However, the measurements for this object may be unreliable.
Indirect distance estimation methods have also been employed. For example, Rigel is believed to be in a region of nebulosity, its radiation illuminating several nearby clouds. Most notable of these is the 5°-long IC 2118 (Witch Head Nebula), located at an angular separation of 2.5° from the star, or a projected distance of 39 light-years (12 parsecs) away. From measures of other nebula-embedded stars, IC 2118's distance is estimated to be 949 ± 7 light-years (291 ± 2 parsecs).
Rigel is an outlying member of the Orion OB1 association, which is located at a distance of up to 1,600 light-years (500 parsecs) from Earth. It is a member of the loosely defined Taurus-Orion R1 Association, somewhat closer at 1,200 light-years (360 parsecs). Rigel is thought to be considerably closer than most of the members of Orion OB1 and the Orion Nebula. Betelgeuse and Saiph lie at a similar distance to Rigel, although Betelgeuse is a runaway star with a complex history and might have originally formed in the main body of the association.
The star system of which Rigel is a part has at least four components. Rigel (sometimes called Rigel A to distinguish from the other components) has a visual companion, which is likely a close triple-star system. A fainter star at a wider separation might be a fifth component of the Rigel system.
William Herschel discovered Rigel to be a visual double star on 1 October 1781, cataloguing it as star 33 in the "second class of double stars" in his Catalogue of Double Stars, usually abbreviated to H II 33, or as H 2 33 in the Washington Double Star Catalogue.
Friedrich Georg Wilhelm von Struve first measured the relative position of the companion in 1822, cataloguing the visual pair as Σ 668. The secondary star is often referred to as Rigel B or β Orionis B. The angular separation of Rigel B from Rigel A is 9.5 arc seconds to its south along position angle 204°. Although not particularly faint at visual magnitude 6.7, the overall difference in brightness from Rigel A (about 6.6 magnitudes or 440 times fainter) makes it a challenging target for telescope apertures smaller than 15 cm (6 in).
At Rigel's estimated distance, Rigel B's projected separation from Rigel A is over 2,200 astronomical units (AU). Since its discovery, there has been no sign of orbital motion, although both stars share a similar common proper motion. The pair would have an estimated orbital period of 24,000 years. Gaia Data Release 2 (DR2) contains a somewhat unreliable parallax for Rigel B, placing it at about 1,100 light-years (340 parsecs), further away than the Hipparcos distance for Rigel, but similar to the Taurus-Orion R1 association. There is no parallax for Rigel in Gaia DR2. The Gaia DR2 proper motions for Rigel B and the Hipparcos proper motions for Rigel are both small, although not quite the same.
In 1871, Sherburne Wesley Burnham suspected Rigel B to be a binary system, and in 1878, he resolved it into two components. This visual companion is designated as component C (Rigel C), with a measured separation from component B that varies from less than 0.1″ to around 0.3″. In 2009, speckle interferometry showed the two almost identical components separated by 0.124″, with visual magnitudes of 7.5 and 7.6, respectively. Their estimated orbital period is 63 years. Burnham listed the Rigel multiple system as β 555 in his double star catalog or BU 555 in modern use.
Component B is a double-lined spectroscopic binary system, which shows two sets of spectral lines combined within its single stellar spectrum. Periodic changes observed in relative positions of these lines indicate an orbital period of 9.86 days. The two spectroscopic components Rigel Ba and Rigel Bb cannot be resolved in optical telescopes but are known to both be hot stars of spectral type around B9. This spectroscopic binary, together with the close visual component Rigel C, is likely a physical triple-star system, although Rigel C cannot be detected in the spectrum, which is inconsistent with its observed brightness.
In 1878, Burnham found another possibly associated star of approximately 13th magnitude. He listed it as component D of β 555, although it is unclear whether it is physically related or a coincidental alignment. Its 2017 separation from Rigel was 44.5″, almost due north at a position angle of 1°.[8] Gaia DR2 finds it to be a 12th magnitude sunlike star at approximately the same distance as Rigel. Likely a K-type main-sequence star, this star would have an orbital period of around 250,000 years, if it is part of the Rigel system.
A spectroscopic companion to Rigel was reported on the basis of radial velocity variations, and its orbit was even calculated, but subsequent work suggests the star does not exist and that observed pulsations are intrinsic to Rigel itself.
Rigel is a blue supergiant that has exhausted the hydrogen fuel in its core, expanded and cooled as it moved away from the main sequence across the upper part of the Hertzsprung–Russell diagram. When it was on the main sequence, its effective temperature would have been around 30,000 K. Rigel's complex variability at visual wavelengths is caused by stellar pulsations similar to those of Deneb. Further observations of radial velocity variations indicate that it simultaneously oscillates in at least 19 non-radial modes with periods ranging from about 1.2 to 74 days.
Estimation of many physical characteristics of blue supergiant stars, including Rigel, is challenging due to their rarity and uncertainty about how far they are from the Sun. As such, their characteristics are mainly estimated from theoretical stellar evolution models. Its effective temperature can be estimated from the spectral type and color to be around 12,100 K. A mass of 21±3 M☉ at an age of 8±1 million years has been estimated by comparing evolutionary tracks, while atmospheric modeling from the spectrum gives a mass of 24±8 M☉.
Although Rigel is often considered the most luminous star within 1,000 light-years of the Sun, its energy output is poorly known. Using the Hipparcos distance of 860 light-years (264 parsecs), the estimated relative luminosity for Rigel is about 120,000 times that of the Sun (L☉), but another recently published distance of 1,170 ± 130 light-years (360 ± 40 parsecs) suggests an even higher luminosity of 219,000 L☉. Other calculations based on theoretical stellar evolutionary models of Rigel's atmosphere give luminosities anywhere between 83,000 L☉ and 363,000 L☉, while summing the spectral energy distribution from historical photometry with the Hipparcos distance suggests a luminosity as low as 61,515±11,486 L☉.
A 2018 study using the Navy Precision Optical Interferometer measured the angular diameter as 2.526 mas. After correcting for limb darkening, the angular diameter is found to be 2.606±0.009 mas, yielding a radius of 74.1+6.1−7.3 R☉. An older measurement of the angular diameter gives 2.75±0.01 mas, equivalent to a radius of 78.9 R☉ at 264 pc. These radii are calculated assuming the Hipparcos distance of 264 pc; adopting a distance of 360 pc leads to a significantly larger size. Older distance estimates were mostly far lower than modern estimates, leading to lower radius estimates; a 1922 estimate by John Stanley Plaskett gave Rigel a diameter of 25 million miles, or approximately 28.9 R☉, smaller than its neighbor Aldebaran.
Due to their closeness to each other and ambiguity of the spectrum, little is known about the intrinsic properties of the members of the Rigel BC triple system. All three stars seem to be near equally hot B-type main-sequence stars that are three to four times as massive as the Sun.
Stellar evolution models suggest the pulsations of Rigel are powered by nuclear reactions in a hydrogen-burning shell that is at least partially non-convective. These pulsations are stronger and more numerous in stars that have evolved through a red supergiant phase and then increased in temperature to again become a blue supergiant. This is due to the decreased mass and increased levels of fusion products at the surface of the star.
Rigel is likely to be fusing helium in its core. Due to strong convection of helium produced in the core while Rigel was on the main sequence and in the hydrogen-burning shell since it became a supergiant, the fraction of helium at the surface has increased from 26.6% when the star formed to 32% now. The surface abundances of carbon, nitrogen, and oxygen seen in the spectrum are compatible with a post-red supergiant star only if its internal convection zones are modeled using non-homogeneous chemical conditions known as the Ledoux Criteria.
Rigel is expected to eventually end its stellar life as a type II supernova. It is one of the closest known potential supernova progenitors to Earth, and would be expected to have a maximum apparent magnitude of around −11 (about the same brightness as a quarter Moon or around 300 times brighter than Venus ever gets). The supernova would leave behind either a black hole or a neutron star.
Installation view of Re:Position.
Harbourfront Centre.
April 20 – June 16, 2013
Photography: Tom Bilenkey
Strategically positioned on a corner that overlooks Clapham Common you shall find No 32 Old Town. Occupying the former site of The Frog, as far as we can see, the transition from boozer to bar restaurant has been seamless. French windows thrown open onto the street and a glorious roof terrace give No 32 a sense of space that turns out to be just perfect on a sunny day. Letâs see how it fares in winter.
As for ambiance - No 32 have gone for the filament lighting, open kitchens and 'stuff with tiles' that seems to be so popular these days. Theyâre quite keen to be seen as a âbar that does good foodâ (as oppose a ârestaurant that does good drinkâ), which is true in the sense that the restaurant area itself is quite small, most of the venue's floor plan is devoted to something that looks more like a pub. Itâs actually quite a lot bigger than it looks from the outside.
How about the food? In the words of another reviewer, No 32âs menu âplays it safeâ (on the main part) - focusing on pub staples such as burgers and steak - but there are a few notable curveballs it may be worth trying out (i.e the âWonky Vegâ Aubergine Curry or the Coconut Poached Chicken Salad). As for drinks, theyâve a very respectable wine list, an OK cocktail list (that focuses quite heavily on Old Fashioned) and a beer list that falls short on their promise of craft beer.
All in all, this place appears to have a very bright future ahead of it - the place was absolutely heaving around 8pm on a Thursday evening. Naaaaice.
Czech swordfighter group "Fictum" at medieval market in Weil am Rhein, 10.06.2007
Nikon D80
Objektiv: SIGMA 70-300mm 1/4-5.6 D
Brennweite: 70mm
Belichtungssteuerung: Zeitautomatik
Belichtungsmessung: Mehrfeld
1/1000 Sekunde(n) - 1/4
Belichtungskorrektur: 0 LW
Empfindlichkeit: ISO 100
Optimierung: Normal
Weißabgleich: Automatik
AF-Betriebsart: AF-A
The Finale to the BARC Club Car Championships Weekender at Brands Hatch and after a Very Thrilling set of both Qualifying Sessions and Races which took place on the Saturday it was Time once again for each Driver to strap in and get ready for some high speed Racing Action thought the Sunday.
In Tribute to the Marshall who was Tragically Killed on the Saturday Some Car and Driver Pairings were Racing with Orange Hearts on their Cars as a Tribute to all of Motorsports Family of Marshalls for who without Racing would not be possible. Thank You!
So Lets get started and see what the days events Haver to Offer and who can Push their Machinery to the Limits and beyond for a Victory.
Britcar Endurance Championship - Trophy Category (Race 1 Results FINAL)
The Britcar Endurance Trophy was the First up and it was time to see who could claim that elusive Pole Position and to see if anyone else could challenge the Top Three Drivers Lets see how things turned out.
In First Place was the Pairing Of (Datum Motorsport's Axel Van Nederveen and Adriano Medeiros) in their Ginetta G55A with a Best Lap Time of 52:193 and an Average Speed of 64.75mph. Congratulations Axel and Adriano a Really Fantastic Drive and A Super Victory.
In Second Place was (SVG's Mark Lee) in his Ginetta G56A with a Best Lap Time of 52.086 and an Average Speed of 64.70mph. Amazing Drive Mark Keeping that Ginetta on the Track and Taking Second Place while Nearly Matching the Speed of Axel and Adriano. Well Done.
In Third Place was (Terry Stephens) in his Peugeot 308 with a Best Lap Time of 53.421 and an Average Speed of 64.50mph. Well Fought Terry a Fantastic Finish in Third Place and Staying Ahead by just over 11 seconds to the Pair of Jasver and Bryan in 4th. Amazing Job.
A Really Enjoyable and Exciting First Race of the Sunday with High Speed Action and Incredible Victories on Track. Congratulations Axel Adriano Mark and Terry. Lets see what Race 2 Brings in terms of the Action.
Britcar Endurance Championship - Trophy Category (Race 2 Results FINAL)
Race 2 For Britcar Next and after a Very Fast and Action Packed First Race Will we see a New Face on the Top Step of the Podium? Lets find out.
In First Place was the Pairing of (Woodrow Motorsport's Simon Baker and Kevin Clarke) in their BMW 1 Series with a Best Lap Time of 51.837 and an Average Speed of 78.22mph. Amazing work Simon and Kevin who have Beaten the Pairing Of (Datum Motorsport's Axel Van Nederveen and Adriano Medeiros) to Victory. An Incredible Drive by Both of them Well Done.
In Second Place was (SVG Mark Lee) in his Ginetta G56A with a Best Lap Time of 52.281 and an Average Speed of 76.89mph. Again a Huge Congratulations to Mark Lee for hanging onto that Second Place Despite Fierce Competition during The Race. Amazing Drive.
In Third Place was (Simon Green Motorsport's Pairing of Jasver Sapra and Brian Branson) in their BMW M3 E46 with a Best Lap Time of 52.718 and an Average Speed of 76.88mph. Congratulations Jasver and Brain Brilliant Drive and well Defended to keep that Third Place in Tact.
Two Incredible Races with Two Very Different Outcomes of Race Winners and Runners Up The Britcar Endurance Trophy is Proving to be Very Competitive this Year.
A Huge Congratulations to Simon Kevin Mark Jasver and Brain for some Amazing Racing and Victories and Good Luck to All Other Drivers. Keep working Hard and Pushing for that All Important Victory.
CTCRC Edmundson Electrical Classic / Historic Thunder Saloons (Race 1 Result FINAL)
Next Up was the CTCRC Electrical and Historic Thunder Saloons and After a Thrilling Qualifying Session Yesterday Lets see what Each Driver has got and who can Push to the Limits for that All Important Victory.
In First Place was (Jason West) in his BMW E46 M3 3200 with a Best Lap Time of 51.907 and an Average Speed of 59.84mph. Congratulations Jason for Another Incredible Drive for First Place and a well Deserved Victory Amongst some Stiff Competition.
In Second Place was (Andrew Wilson) in his Holden Monaro 7000 with a Best Lap Time of 52.418 and an Average Speed of 59.96mph. Well Done Andrew Fantastic Driving and a Super Defensive Drive for Second Place.
In Third Place was (Samuel Wilson) in his Aston Martin V8 Vantage with a Best Lap Time of 52.699 and an Average Speed of 59.50mph. Amazing Work Samuel and a Beautiful Example of the Aston Martin V8 Vantage on Display Showing its Raw Power and Racing Pedigree to Finish in Third Place.
A Fantastic Finish to The Historic and Electrical Thunder Saloons Racing at The Weekend. A Huge Congratulations to Our Top Three Finishers Jason Andrew and Samuel. Fantastic Racing from all Three of you and Good Luck to all other Drivers Keep Tuning and Working Hard and I'm sure Victory Will not be too Far Away from you.
CTCRC JEC Saloon & GT Championship & Burton Power BOSS (Race 2 Results FINAL)
Next Up CTCRC Saloon and GT Championships and with some Fierce Competition on Display during not only Qualifying but also Their First Race on the Saturday Which saw Malcom Harding Storm to an Insane Victory who Will be able to Take him on and Potentially Steal his Crown during the Next Race Today? Lets See.
In First Place was (Malcom Harding) in his Ford Escort MK2 Zakspeed 2500 with a Best Lap Time of 53.888 and an Average Speed of 78.49mph. Another Incredible Victory for Malcom that Highly Modified Zakspeed Escort Really Shows off the Power and Performance of a True Champion and a Fantastic Driver. Congratulations Malcom.
In Second Place was (Steven Goldsmith) in his Ford Anglia 105e 260 with a Best Lap Time of 54.335 and an Average Speed of 78.21mph. Another Storming Drive to Achieve Second Place for Steven. Fantastic Driving and Amazing Car Control through Every Corner. Congratulations Steven.
In Third Place was (Tom Robinson) in his Jaguar XJ6 4000 with a Best Lap Time of 55.481 and an Average Speed of 55.481mph. Congratulations Tom Superb Display of Driving Ability behind the Jag and a Well Deserved Third Place for Him.
Another Incredible Weekend of Racing for the CTCRC Saloon and GT Championships with Some New and Some Old Drivers Stepping onto the Podium. Massive Congratulations to Malcolm Steven and Tom for their First Second And Third Place Finishes. Keep Up the Good Work and Never Stop Trying.
CTCRC Laser Tools Pre 93 & Simply Serviced Pre 03 Touring Cars (Race 1 Results FINAL)
Now Its Time for The Laser Tools Pre 93 and Simply Serviced Pre 03 Touring Cars to make their way back onto The Track for what Looked to be a Spectacular Race. A Whole Range of Different Cars to Race Against and Stiff Competition after Qualifying Proves that This Race will be One not to be Missed. Lets See what Unfolded.
In First Place was (Gary Prebble) in his Honda Civic EG 2000 with a Best Lap Time of 54.100mph and an Average Speed of 78.60mph. Well Done Gary a Really Well Deserved First Place Victory and an Amazing Drive to the Flag.
In Second Place was (David Griffith) in his BMW E36 M3 3058 with a Best Lap Time of 54.558 and an Average of 78.42mph. Incredible Drive their David Pushing that BMW For Everything that it Has got to Achieve Second Place.
In Third Place was (Kam Tunio) in his Honda Civic EK9 1595 with a Best Lap Time of 55.347 and an Average Speed of 77.05mph. Well Driven Kam Super Driving on Display and a Well Deserved Third Place Finish.
Another Amazing Race for The Pre 93 and Pre 03 Touring Cars and a Huge Congratulations to Gary David and Kam for their First Second and Third Place Victories. Keep up the Hard Work and Good Luck to everyone Else wherever your Next Races take you.
CTCRC Poultec Classic Race Engines Pre 66 Touring Cars (Race 1 Results)
Now it was Time for the Fan Favourite to Enter onto the Brands Hatch Circuit with the Pre 66 Touring Cars Championship. With Mini's Lotus Cortina's and Ford Falcons. This was One Race that No One Wanted to Miss. After a Very Fast Paced Qualifying Session on the Saturday Which saw (Alan Greenhalgh) take Pole Position who Will be able to Challenge Him During the Race and Snatch Victory Away from Him.
In First Place was (Alan Greenhalgh) in his Ford Falcon with A Best Lap Time of 58.707 and an Average Speed of 72.63mph. Congratulations Alan A Beautiful Example of the Ford Falcon and Certainly a Very Fast One too. Congratulations on Your Victory.
In Second Place was (Robyn Slater) in his Ford Anglia 1550 with a Best Lap Time of 58.992 and an Average Speed of 72.06mph. Very Good Drive their From Robyn to Secure Second Place in The First Race of the Day for the Pre 66 Touring Cars.
In Third Place was (Barry Sime) in his Morris Mini Cooper S 1293 with a Best Lap Time of 59.116 and an Average Speed of 71.95mph. Fantastic Work their Barry Keeping that Little Rocket on The Track looked to be Very Challenging but A Very Well Deserved Third Place.
What A First Race for The Historic Pre 66 Touring Cars showing The Power and Pride Each Driver takes in Both Racing and Preservation on Their Beloved Racing Machines. Congratulations to Alan Robyn and Barry on their First Second and Third Place Finishes. Lets See what New Challenges Await Them in Race 2 The Final Race of The Day for Them.
CTCRC Poultec Classic Race Engines Pre 66 Touring Cars (Race 2 Results FINAL)
The Epic FINALE To The Pre 66 Touring Cars Race was A Race in Wet Conditions Making it even more Challenging for The Top Three Drivers. Who would Win and be able to Retain if not Take on thease Three Giants of Touring Car Racing in thease Conditions. Lets See How Things Concluded.
In First Place was (Barry Sime) in his Morris Mini Cooper S 1293 with a Best Lap Time of 1:11.482 and an Average Speed of 58.62mph. Amazing Work Barry to take Home a Superb Victory and a Brilliant Bit of Wet Weather Driving in The Mini Well Done.
In Second Place was (John Davies) in his Austin Mini Cooper S 1293 with a Best Lap Time of 1:11.416 and an Average Speed of 58.38mph. Amazing Work John Racing A Mini in thease Conditions is Very Tricky and Yet both You and Barry made it look Easy.
In Third Place was (James Ibbotson) in his Hillman Imp Super 998 with a Best Lap Time of 1:11.518 and an Average Speed of 58.12mph. Well Done James Sliding that Imp around in the Wet for a Magnificent Third Place was Well Deserved.
What A Race to End the Day for the Pre 66 Touring Cars and with So many Old and New Winners Lets Hope we Get to see More Races like This One Thought the Rest of the 2021 Season. A Big Congratulations to Barry John and James on their Respective Victories and Keep Trying Everyone Else The Hard Work will Pay off.
CTCRC Shell Oils Pre 83 Touring Cars (Race 1 FINAL)
Up Next The Pre 83 Touring Cars took to the Track for Their Only Race of The Day and from what We Have Seen Already This Race also looks like its going to be a Very Strong Battle for First Second and Third Place. Lets See who Came First and Took that All Important Victory.
In First Place was (Mark Lucock) in his Ford Escort MK1 RS2000 2040 with a Best Lap Time of 57.687 and an Average Speed of 74.53mph. Amazing work there Mark Pushing All the Power the RS2000 Engine Has and Keeping it on Track to Score an Amazing Victory.
In Second Place was (Stephen Primett) in his Ford Escort MK1 2037 with a Best Lap Time of 57.503 and an Average Speed of 74.52mph. Another Brilliant Drive from the Likes of Stephen Keep the Pace with Mark and Making for some Fierce Competition Thought the Race.
In Third Place was (Mike Luck in his BMW E21 320 1998 with a Best Lap Time of 57.236 and an Average Speed of 74.46mph. Super Driving there Mike to take Third Place and a Very Classic Looking BMW Indeed.
What A Race from the Pre 83 Touring Cars showcasing Speed Power and What a Touring Car was Made to do around a Race Track. A Big Congratulations to Mark Stephen and Mike on their First Second and Third Place Finishes. Keep Racing and Keep Having Fun Out There.
Junior Saloon Car Championship (Race 1 Result FINAL)
The Junior Saloon Car Championship was Up Next and Even Though the Age Range of thease Next Drivers Taking to the Circuit Might Shock you at The Fact that Many of them are as Young as 15 Years of age don't be Fooled Because thease Guys Know how to Race Having been brought up from Carting since the age of 4. They are always a Fan Favourite and After Qualifying on the Saturday its Anyone's Game as to Who Wins and Who Losses in Thease Races.
In First Place was (Ruben Hage) in his Citroen Saxo VTR 1600 with a Best Lap Time of 59.967 and an Average Speed of 65.65mph. Congratulations Ruben What A Drive and an Incredible Run for First Place Fending off the Other On Coming Drivers. Truly a Championship Winning Drive.
In Second Place was (Harvey Caton) in his Citroen Saxo VTR 1600 with a Best Lap Time of 59.629 and an Average Speed of 65.64mph. Very Well Driven there Harvey Staying very Close to Ruben in First Place and Keeping Him on His Toes Thought the Entire Race.
In Third Place was (Charlie Hand) in his Citroen Saxo VTR 1600 with a Lap Time of 1:00.006 and an Average Speed of 65.57mph. Solid Third Place there Charlie Keep Up the Momentum and Never Give Up Chasing Your Dreams.
What a Fantastic Race from the Junior Saloon Car Championship with New Winners on the Podium and Some Close Wheel to Wheel Action Thought the Race Thease Guys will be Fantastic To see in Future Racing Series All Over The World. Congratulations to Ruben Harvey and Charlie for First Second and Third Place and Good Luck to All Other Aspiring Young Drivers Following in the Footsteps of Your Greatest Racing Heroes.
Kumho BMW Championship (Race 1 Results)
Finally it was Time for the Last Two Races of the Day the Kumo BMW Championship. Featuring The Makes and Models of Many BMW'S taking to the Circuit for Race 1. After a Busy Day Qualifying on Saturday Lets See what Each Driver Cando in The Frist of Two Races for their Championship.
In First Place was (Niall Bradley) in his BMW E46 M3 with a Best Lap Time of 50.920 and an Average Speed of 83.60mph. Brilliant Driving There Niall Pushing the Power of the BMW Engine to Max and Putting the Pedal to the Metal the Whole Race. A Superb Victory.
In Second Place was (Michael Vitulli) in his BMW E36 M3 3200 with a Best Lap Time of 51.158 and an Average Speed of 83.45mph. Another Incredible Driver Pushing Hard and Taking Second Place. Well Done Michael.
In Third Place was (James Card) in his BMW E46 M3 3200 with a Best Lap Time of 51.154 and an Average Speed of 83.42mph. Very Well Done their James Keep Pushing.
Three Fantastic Drivers in Niall Michael and James all Fighting for that Victory and Showing The Racer Inside each and Everyone of them. Lets see what Their Final Race of the Day Brings Them.
Kumho BMW Championship (Race 2 Results FINAL)
In First Place was (Niall Bradley) in his BMW E46 M3 with a Best Lap Time of 53.581 and an Average Speed of 77.79mph. Another Well Deserved First Place Finish to Round of The Days Racing. Congratulations Niall Go and Celebrate with The Team In Style.
In Second Place was (Darren Morgan Owen) in his BMW E46 M3 3200 with a Best Lap Time of 53.200 and an Average Speed of 77.43mph. Super Drive There Darren for Second Place and a New Winner onto The Podium.
In Third Place was (Brad Sheean) in his BMW E46 M3 3200 with a Best Lap Time of 53.227 and an Average Speed of 77.13mph. Fantastic Drive there Brad and Some Incredible Car Control thought the Entire Race to Finish Third.
And That Concludes Racing for the Kumho BMW Championship with 4 Different Winners Across two Races and A lot of Really Fast Action you could not Have Asked for a better Finish to The End of The Days Racing. Massive Congratulations to Niall Darren and Brad and Good Luck to all Other Competing Drivers who are still Looking for that almighty Victory.
That Concludes Racing for The BARC Club Car Championships Weekend A Big Congratulations to All of the Drivers of Every Team and a Huge Thank You to Marshalls Far and Wide as Without Your Support Events like This and Champion Drivers May Never Get to Achieve Their Dreams.
See You All At The Next One!
Positioned along track to Church Farm, this FW3/28 Type 28 anti-tank gun house is sited facing north to defend the river crossing at Jude's Ferry Bridge. The gun emplacement was fitted with a pedestal and nine-bolt holdfast for a 6-pounder anti-tank gun.
The FW3/28 Type 28 is a rectangular shellproof gun house designed to house either a 2pdr or 6pdr Hotchkiss anti-tank gun. The smallest Type 28 gun house, is a single chamber design built to a shellproof standard, with external walls approximately 3ft 6in thick whilst the roof is 12in thick. Overall it approximately measures 20ft by 19ft and internally the chamber measures 13ft by 12ft. At the front of the Type 28 gun house is the low and wide embrasure for the 2pdr or 6pdr anti-tank gun. With the 2pdr gun in position the shield of the gun would have covered most of the embrasure, which measures 2ft 6in internally, stepping out to 3ft 2in by 11ft 6in on the outside, the maximum traverse of the 2pdr gun was limited to a 60° sweep.
Getting the 2pdr gun inside the gun house was through a rear opening of 6ft wide, which would be closed in with sandbags as there were no doors fitted. The large unobstructed entrance did allow the 2pdr gun to maintain it’s mobility, by allowing the gun to be moved in and out rapidly. Below the gun embrasure are three recesses in the floor, the 2pdr gun, would have been wheeled into position, then its wheels removed and the trail legs unfolded and located into the floor recesses. In cases were the Hotckiss quick fire anti-tank gun was used a pedestal with a nine bolt holdfast was added to mount the gun, in a more permanent position adding sandbags around the embrasure for added protection.
Normally each side wall has an infantry embrasure, to provide some limited protection from the enemy. However, the lack of all-round small arms fire meant that the gun house would be very vulnerable to enemy attack. The lack of forward-firing Infantry embrasures meant that it would not be possible to support the 2pdr gun with small arms fire. So to overcome the problem of the limited infantry fire support the FW3/28 gun house design was modified to produce the FW3/28a. This modification consisted of a second chamber being added to the anti-tank gun chamber, the second chamber was an infantry chamber with up to three infantry embrasures, firing to the front, rear and side. Generally, the gun houses were positioned to allow the gun to fire along fixed lines, such as enfiladingss an anti-tank ditch or a bridge. In these positions the limited traverse of the gun creates no real disadvantage and the small size of the embrasure provides greater protection for the gun and its crew.
Eastern Command: Corps and Command Stop Lines – One of three Eastern Command Corps stop lines, this one running from the River Colne in Essex via Wakes Colne and Bures, along the River Stour to Sudbury and Long Melford, and thence to Bury St. Edmunds and the River Lark at Mildenhall. Its final stretch (known now as the Command Line) was via Littleport along the line of the River Great Ouse to King's Lynn.