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Thursday, March 27, 2025

Dwarf

Dwarf (pronounced dwawrf)

(1) A person of abnormally small stature owing to a pathological condition, especially one suffering from cretinism or some other disease that produces disproportion or deformation of features and limbs.  In human pathology, dwarfism is usually defined, inter-alia, as an adult height less than 1.47 m (4 ft 10 in).

(2) In zoology & botany, an animal or plant much smaller than the average of its kind or species.

(3) In European folklore, a being in the form of a small, often misshapen and ugly, man, usually having magic powers.

(4) In Norse mythology, any member of a race of beings from (especially Scandinavian and other Germanic) folklore, usually depicted as having some sort of supernatural powers and being skilled in crafting and metalworking, often as short with long beards, and sometimes as clashing with elves.

(5) In astronomy, a small version of a celestial body (planet, moon, galaxy, star etc).

(6) Of unusually small stature or size; diminutive; to become stunted or smaller.

Pre 900: From the Middle English dwerf, dwergh, dwerw & dwerȝ, from the Old English dweorh & dweorg (dwarf), replacing the Middle English dwerg and ultimately from the Proto-Germanic dwergaz.  It was cognate with the Scots dwerch, the Old High German twerg & twerc (German Zwerg), the Old Norse dvergr (Swedish dvärg), the Old Frisian dwirg (West Frisian dwerch), the Middle Low German dwerch, dwarch & twerg (German & Low German Dwarg & Dwarch) and the Middle Dutch dwerch & dworch (Dutch dwerg).  The Modern English noun has undergone complex phonetic changes. The form dwarf is the regular continuation of Old English dweorg, but the plural dweorgas gave rise to dwarrows and the oblique stem dweorge which led to dwery, forms sometimes found as the nominative singular in Middle English texts and in English dialects.  Dwarf is a noun and verb, dwarfness & dwarfishness are nouns, dwarfish & dwarflike are adjectives and dwarfishly is an adverb.  The plural forms are dwarves and dwarfs.  Dwarfs was long the common plural in English but after JRR Tolkien (1892-1973) used dwarves, his influence was enough to become the standard plural form for mythological beings.  For purposes non-mythological, dwarfs remains the preferred form.

The M Word

1972 MG Midget (RWA) in British Racing Green (BRG).

Dwarf seems still to be an acceptable term to describe those with dwarfism and Little People of America (LPA), the world’s oldest and largest dwarfism support organization (which maintains an international, membership-based organization for people with dwarfism and their families) has long campaigned to abolish the use of the word “midget” in the context of short humans.  The objection to midget is associative.  It was never part of the language of medicine and it was never adopted as official term to identify people with dwarfism, but was used to label used those of short stature who were on public display for curiosity and sport, most notoriously in the so-called “freak shows”.  Calling people “midgets” is thus regarded as derogatory.  Midget remains an apparently acceptable word to use in a historic context (midget submarine, MG Midget et al) or to describe machinery (midget car racing; the Midget Mustang aerobatic sports airplane) but no new adoptions have been registered in recent years.  The LPA is also reporting some supportive gestures, noting with approval the decision of the Agricultural Marketing Service (AMS) of the US Department of Agriculture’s (USDA) to revise the nomenclature used in the US standards for grades of processed raisins by removing five references to the term “midget”.  Although obviously a historically benign use of the word, its removal was a welcome display of cultural sensitivity.

An interesting outlier however is midget wrestling, a field in which the participants are said enthusiastically to support the label, citing its long traditions and the marketing value of the brand.  Although in the late twentieth century, midget wrestling’s popularity diminished in the last decade there’s be a resurgence of interest and the sport is now a noted content provider for the streaming platforms which run live and recorded footage.  Since the 1970s, midget wrestling has included styles other than the purely technical form with routines extending from choreographed parody and slapstick performances to simulated sexual assault.  These innovations have attracted criticism and the suggesting it’s a return to the freak shows of earlier centuries but audiences in the target demographic seem appreciative and, noting the success of a number of tours and operators, Major League Wrestling in 2022 announced the creation of a midget division.

The MG Midget

Where it began: 1930 MG M-Type Midget Roadster.

The earliest cars to wear MG badge (the name originally “Morris Garages”, an operation which had the same relationship to Morris as AMG does to Mercedes-Benz (ie high-performance variants)) were tuned (and often re-bodied) editions of existing Morris models but in 1928 the 8/33 M.G Midget Sports Series M (truncated usually to “M Type” was displayed at the 1928 London Olympia Motor, series production commencing the next season.  The first of a long line of tiny roadsters, 3,232 would be made between 1929-1932 and the one in the photographs above is fitted with coachwork typical of the era: an open two-seater in the fashionable “boat-tail” style, constructed by Carbodies of Coventry using construction technique which began in aviation, the panels a mix of steel and fabric-covered plywood over an ash frame.  The fabric soft-top was stored under the rear deck along its frame, tools and a spare wheel.  In the spirit of the age, a rakish two-piece windshield was fitted and there was no provision for a heater.  Despite the minimalist accommodation, the engine was surprisingly advanced, the four-cylinder engine using a bevel-gear-driven single overhead cam turning off the vertically mounted generator, 27 horsepower at a then impressive 5400 rpm generated from a displacement of 847 cm3 (51.68 cubic inches).  A footnote in the Midget’s history is that the first exported to the US was in 1930 bought by Edsel Ford (1893–1943; president of the Ford Motor Company (FoMoCo) 1919–1943), then titular head of his father’s (Henry Ford (1863-1947)) eponymous Motor company which, by the million, built larger vehicles.

1960 Austin-Healey Sprite Mark I (top left), 1966 MG Midget Mark II (top right), 1973 MG Midget Mark III (RWA, bottom left) and 1979 MG Midget Mark IV (bottom right).

For a new generation (1961-1979) of diminutive roadsters, MG revived the Midget name last used on the M-Type. MG was by the 1950s part of British Motor Corporation (BMC (1952-1967) which later would be absorbed by the doomed British Leyland (1968–1990)) and a corporate companion marquee was Austin-Healey which between 1958-1961 produced the Sprite (known variously as the “bugeye” or “frogeye”), a small sports car, built on the familiar template of economy car underpinnings with a stylish body.  After the release of the MGA (1955-1962), MG no longer had a competitor in the low-price segment so BMC took the decision that the two companies would share the model, yet another example of the “badge engineering” which BMC pragmatically (and for a while lucratively) would exploit until the process descended into self-defeating absurdity.  When the Mark II Sprites were released in 1961 (without the distinctive headlights which were the source of the nicknames), simultaneously there was the debut of the Midget, the latter slightly more expensive and better equipped, although both remained basic roadsters in the old tradition, lacking fittings such as side windows and external door-handles.  The Sprite would continue in three versions (Mark II; 1961-1964, Mark III; 1964-1966, Mark IV 1966-1971) before, following the end of BMC’s contractual arrangement with Donald Healey (1898–1988), briefly it was sold as the Austin Sprite (1971-1972) before the name was retired and the segment was left to MG.  In the decade they’d been companion models, the pair significantly had been improved, gaining power, refinement and creature comforts (the overdue door handles and side windows part of the Mark II upgrades) but what never changed were the dimensions, the things always small, something the balanced styling tended to disguise, the compactness best appreciated when one was seen parked next to a more typically sized vehicle; the Sprite and Midget being dwarfed.

Almost 130,000 Sprites were built while Midget production (which lasted until 1980) totalled some 225,000, the most numerous being the later models (Mk III; 1966–1974: 100,246 units & 1500; 1974–1979: 81,916 units).  A decade before production ended it was already outdated but such was the charm (and lack of competition) that demand remained strong almost to the end.  The most fancied Midgets are the so-called RWA (round wheel arch) models produced between 1972-1974; these adopted the design used on the rear of the bugeyes and are considered the best looking (as well as making the use of wider rear tyres easier) but in 1974 MG had to revert to the squared-off look because the strength gain from the additional metal was necessary to support the large “rubber” bumpers added to conform with US regulations; the RWA bodywork was found to be prone to damage when the rear-impact tests were conducted.  Even before the huge bumpers unhappily had been grafted, US market cars had for some months had large rubber “buffers” bolted to the chrome bumpers, known in the US as “Dagmars” and in the UK as “Sabrinas” both names tributes to the hardly vague anatomical similarity with the two pop culture figures.  Along with the big bumpers, to comply with minimum headlight height regulations in the US, the suspension height was raised by about an inch (25 mm), something which raised the centre of gravity and thus affected the handling characteristics, something adjustments to the anti-roll bars only partially ameliorated.  Visually, the increased height was disguised by lowering curve of the front wheel arch.

Triumph Spitfire, also a midget-sized roadster

A midget (with a small “m”) dwarfed by two behemoths: A 1977 Triumph Spitfire between two Ford Super Duty F-450s heavy pick-up trucks.  At their intended purpose (carrying or towing heavy payloads) Ford’s Super Duty heavy pick-up trucks perform well but such is the consumer appeal they’re a not uncommon sight used as passenger vehicles, even in cities; they can thus be both a personal and political statement, owners delighted Ford has made pick-ups great again (MPUGA).

Adopted for the range in 1999, Ford between 1958-1981 had previously used the “Super Duty” label on three large displacement (401, 477 & 534 cubic inch (6.6, 7.8 & 8.8 litre) gas (petrol) V8s, the family one of a remarkable variety of different V8s the corporation produced during the 1950s & 1960s.  Big, heavy and low-revving, the Super Duty V8 were legendarily robust and famed for their longevity but were doomed ultimately by their prodigious thirst.  They were intended only for heavy-duty, industrial use and in that very different from the Pontiac Super Duty (SD) V8s which were high-performance units, the early versions in the 1960s optimized for drag racing while the revival the next decade was the final fling of the original muscle car era (1964-1974).  The 389 & 421 cubic inch (6.4 & 6.9 litre) versions were offered between 1960-1963 while the 455 (7.5) appeared in 1973-1974 and had it not been for the 455 SD Pontiac Firebirds in those years, the muscle car era would have been regarded as having ended in 1972.  The Watergate-era 455 SD is also a footnote in the history of environmental law because Pontiac (in a preview of Volkswagen’s later “Dieselgate”) used a device to “cheat” on emission testing being undertaken as part of the certification process.  Caught re-handed, Pontiac, guilty as sin, was compelled to remove the “cheat gear” and re-submit a vehicle for testing; that’s the reason the 1973-1974 455 SD was rated at 290 horsepower (HP) rather than the 310 of the original (and more toxic) engine.

1967 Triumph Spitfire Mark II (left) and 1972 Triumph Spitfire Mark IV (with after-market exhaust tips, right).

The Triumph Spitfire had the same relationship to the larger TR sports cars (1952-1976) as the Midget did to the MGB.  Produced in five distinct generations between 1962-1980, like the Sprite & Midget, the Spitfire featured a stylish body atop the platform of a high-volume model and for the coachwork Triumph out-sourced the job to Italy, Giovanni Michelotti (1921–1980) producing a shape which owed nothing to the little Herald (1959-1971) on which it was based.  In continuous production in five versions (Mark I; 1962–1964, Mark II; 1965–1967, Mark III; 1967–1970, Mark IV; 1970–1974 & 1500; 1974–1980), almost 315,000 were built with the later models the most popular, the some 96,000 of the 1500s sold.  Like the Midget, the Spitfire was over the years improved although the things did at least stagnate in the post-1974 US models which became heavier, slower and uglier although in the 1970s that was a general industry trend.  The Although soon under the same corporate umbrella, the Midget & Spitfire were competitors (in the showroom and on the circuits) for almost two decades and when Road & Track magazine in their September 1967 edition published a comparison test, they couldn't decide which was best, concluding: "...whichever one the buyer chooses, he is assured of many miles of motoring pleasure in the great sports car tradition.  They're good cars, both of them.  You can't go wrong."  For the readers that may not have been a great deal of help and the phrasing must have been force of habit because the two little roadsters had always enjoyed some popularity among women.  

The photograph run in 1959 with the caption “Hark the Herald’s axle’s swing” (left) and a Mark I Spitfire's swing axles displaying the same behavior.

The Spitfires of the 1960s were a bit more lively but that description wasn’t always a compliment because, based on the Herald, what was inherited was the swing-axle rear suspension and swing the axles certainly could, leading to a “lively rear”.  When the British motoring press first tested the Herald they noted the behaviour of the swing axles under extreme load and had a photographer appropriately positioned: The caption “Hark the Herald’s axle’s swing” became famous.  None of that deterred Triumph which in 1962 introduced a more powerful version powered by a 1.6 litre (97 cubic inch) straight six.  That meant a faster car which meant the behaviour of the swing axles could be experienced at a higher speed (with all that implies) but the car sold well which was encouraging so Triumph in 1966 fitted a 2.0 litre (122 cubic inch) six.  It was not until 1968 the rear suspension was revised and this curative solved the errant characteristics to a degree which impressed even the usually sceptical motoring journalists and sales remained strong until production ended in 1971.  Offered only in four-cylinder form, the revisions to the Spitfire’s rear suspension were less complex but when tested on the Mark IV in 1970, the improvement was apparent and from this point, criticism ceased of of road-holding at the limit.

1967 Triumph GT6 Mark I (also with after-market exhaust tips, left) and 1979 Triumph Spitfire 1500 (right).  With production ending in 1973, the GT6 was spared from being disfigured by the battering-ram like bumpers imposed on the Spitfire, those on the last of the line (1979-1980) the biggest.

While the roadster never gained six-cylinder power, Triumph from 1966 offered a coupé version (with a convenient hatchback, al la the Jaguar E-Type (XKE, 1961-1974) called the GT6.  Mechanically it followed the Vitesse except it was only ever fitted with the 2.0 litre engine and didn’t receive the suspension fix until the Mark II in 1969 and that transformed things although, being relatively complex it must have been deemed too expensive to justify on what proved a low-volume model and the with the release of the Mark III in 1970, a version of that used on the Spitfire was substituted and it proved just as effective.  Sales of the GT6 never matched the company’s expectation and the market preferred the MGB GT (1965-1980) which used the same concept for the body.  Noting the costs which would have been incurred to make the GT6 compliant with the US regulations to take effect from 1974, production ended in late 1973.  Because the considerably more powerful (especially the fuel-injected versions sold outside the US) 2.5 litre six Triumph used in the TR5 (which, with twin carburetors, was in North America sold as the TR-250), TR6, 2.5 PI & 2500 is a relatively easy swap, quite a few GT6s have been so upgraded although some attention does need to be paid to the chassis to achieve a completely satisfactory road car.  

The short stature of Victor Emmanuel III (1869–1947; King of Italy 1900-1946) with (left to right), with Aimone of Savoy, King of Croatia (Rome, 1943), with Albert I, King of the Belgians (France, 1915), with his wife, Princess Elena of Montenegro (Rome 1937) & with Adolf Hitler (1889-1945; Führer (leader) and German head of government 1933-1945 & head of state 1934-1945), observing the Italian navy conduct manoeuvres, Gulf of Naples, 1938.  Note the King of Italy's sometimes DPRKesque hats.

Technically, Victor Emmanuel didn’t fit the definition of dwarfism which sets a threshold of adult height at 4 feet 10 inches (1.47 m), the king about 2 inches (50 mm) taller (or less short) and it’s thought the inbreeding not uncommon among European royalty might have been a factor, both his parents and grandparents being first cousins.  However, although not technically a dwarf, that didn’t stop his detractors in Italy’s fascist government calling him (behind his back) il nano (the dwarf), a habit soon picked up the Nazis as der Zwerg (the dwarf) (although Hermann Göring (1893–1946; leading Nazi 1922-1945, Hitler's designated successor & Reichsmarschall 1940-1945) was said to have preferred der Pygmäe (the pygmy)).  In court circles he was knows also (apparently affectionately) as la piccola sciabola (the little sabre) a nickname actually literal in origin because the royal swordsmith had to forge a ceremonial sabre with an unusually short blade for the diminutive sovereign to wear with his many military uniforms.  His French-speaking wife (Princess Elena of Montenegro (1873–1952; Queen of Italy 1900-1946)) stood a statuesque six feet (1.8 m) tall and always called him mon petit roi (my little king).  It was a long and happy marriage and genetically helpful too, his son and successor (who enjoyed only a brief reign) very much taller although his was to be a tortured existence Still, in his unhappiness the scion stood tall and that would have been appreciated by the late Prince Philip, Duke of Edinburgh (1921–2021) who initially approved of the marriage of Lady Diana Spencer (1960-1997) to the Prince of Wales (b 1948) on the basis that she “would breed some height into the line”.

In cosmology, the word dwarf is applied to especially small versions of celestial bodies.  A dwarf galaxy is a small galaxy of between several hundred and several billion stars, (the Milky Way may have as many as billion) and astronomers have identified many sub-types of dwarf galaxies, based on shape and composition.  A dwarf planet is a small, planetary-mass object is in direct orbit of a star, smaller than any of the eight classical planets but still a world in its own right.  Best-known dwarf planet is now Pluto which used to be a planet proper but was in 2006 unfortunately down-graded by the humorless types at the International Astronomical Union (IAU) who are in charge of such things.  It’s hoped one day this decision will be reversed so Pluto will again be classified a planet.  Dwarf planets are of interest to planetary geologists because despite their size, they may be geologically active bodies.  The term dwarf star was coined when it was realized the reddest stars could be classified as brighter or dimmer than our sun and they were created the categories “giant star” (brighter) and dwarf star (dimmer).  As observational astronomy improved, the

With the development of infrared astronomy there were refinements to the model to include (1) the dwarf star (the “generic” main-sequence star), (2) the red dwarf (low-mass main-sequence star), (3) the yellow dwarfs are (main-sequence stars with masses comparable to that of the Sun, (4) the orange dwarf (between a red dwarf and yellow/white stars), (5) the controversial blue dwarf which is a hypothesized class of very-low-mass stars that increase in temperature as they near the end of their main-sequence lifetime, (6) the white dwarf which is the remains of a dead star, composed of electron-degenerate matter and thought to be the final stage in the evolution of stars not massive enough to collapse into a neutron star or black hole, (7) the black dwarf which is theorized as a white dwarf that has cooled to the point it no longer emits visible light (it’s thought the universe is not old enough for any white dwarf to have yet cooled to black & (8) the brown dwarf, a sub-stellar object not massive enough to ever fuse hydrogen into helium, but still massive enough to fuse deuterium.

Coolest dwarf of all is (9) the ultra-cool dwarf (first defined in 1997), somewhat deceptively named for non cosmologists given the effective temperature can be as high as 2,700 K (2,430°C; 4,400°F); in space, everything is relative.  Because of their slow hydrogen fusion compared to other types of low-mass stars, their life spans are estimated at several hundred billion years, with the smallest lasting for about 12 trillion years.  As the age of the universe is thought to be only 13.8 billion years, all ultra-cool dwarf stars are relatively young and models predict that at the ends of their lives the smallest of these stars will become blue dwarfs instead of expanding into red giants.

Disney's seven dwarfs; they're now cancelled.

The events towards the conclusion of the nineteenth century German fairy tale Snow White and the Seven Dwarfs make ideal reading for young children.  Her evil step-mother has apparently killed poor Snow White so the seven disappointed dwarfs lay her body in a glass coffin.  The very next, a handsome prince happens upon the dwarfs’ house in the forest and is so captivated by her beauty he asks to take her body back to his castle.  To this the dwarfs agree but while on the journey, a slight jolt makes Snow White come to life and the prince, hopelessly in love, proposes and Snow White accepts.  Back at the palace, the prince invites to the wedding all in the land except Snow White's evil stepmother.

Snow White and the Seven Dwarfs, even Happy looking sad.

The step-mother however crashes the wedding and discovers the beautiful Snow White is the bride.  Enraged, she again attempts murder but the prince protects her and, learning the truth from his bride, forces the step-mother to wear a pair of red-hot iron slippers and dance in them until she dies; that takes not long and once she has the decency to drop dead, the nuptials resume.  In the way things happen in fairy tales, the prince and Snow White live happily ever after.

DEI (diversity, equity and inclusion)

The condition achondroplasiaphobia describes those with a “fear of little people".  The construct is achondroplasia (the Latin a- (not) +‎ the Ancient Greek chondro- (cartilage) + the New Latin‎ -plasia (growth); the genetic disorder that causes dwarfism) + phobia (from the New Latin, from the Classical Latin, from the Ancient Greek -φοβία (-phobía) from φόβος (phóbos) (fear).  The condition, at least to the extent of being clinically significant, is thought rare and like many of the especially irrational phobias is induced either by (1) a traumatic experience, (2) depictions in popular culture or (3) reasons unknown.  Achondroplasiaphobia has never appeared in the American Psychiatric Association’s (APA) Diagnostic and Statistical Manual of Mental Disorders (DSM).  In 2006, it was reported that while dining at the Chateau Marmont hotel in Los Angeles, after noticing two people of short stature had entered the restaurant, Lindsay Lohan suffered an "anxiety attack" and hyperventilated to the extent she had to take "an anti-anxiety pill" to calm down.  To her companions she repeatedly said "I’m so scared of them!"  A spokesperson for the LPA responded by suggesting Ms Lohan should "...treat her fear the same as she would a fear of any other protected minority population.  If that fails, she might find diversity training to be useful."  Almost immediately the story appeared, it was debunked by a representative for Ms Lohan who issued a statement  saying she is not achondroplasiaphobic and not in any way scared of little people, adding "Lindsay loves all people."

Prince Charming's non-consensual kiss of Snow White on her "lips red as blood".

In February 2025, Luis Rubiales (b 1977), the former president of the Royal Spanish Football Federation was found guilty of sexual assault for kissing player Jenni Hermoso (b 1990) without her consent and was fined €10,800 so, at least in some jurisdictions, the matter of consenting to a kiss is not mere legal theory.

Among critics and industry analysts, the consensus seem to be that in late 1919 when the project was approved, for Disney to allocate a budget of US$200 million (it ended up being booked at around US$250 million) to a remake of Snow White and the Seven Dwarfs (1937) probably was a good idea.  Based on the German fairy tale Sneewittchen which first appeared in print early in the nineteenth century, Disney’s 1937 production was the first animated, full-length feature film made in the US and it was both critically acclaimed and a great commercial success, becoming the highest-grossing film of 1938; adjusted for inflation, it’s success then and since has made it one of the most profitable films ever made.

The elements in its success were (1) the quality of the studio’s work, (2) advances in the technology delivering sight and sound which made the audience's experience so vivid and (3) the threads of the story which are fairy tale classics: A wicked queen, jealous of her stepdaughter’s beauty orders her murder, only to discover she’s hiding out in a cottage with seven dwarves so she poisons her with an adulterated apple, inducing a deep sleep from which she eventually is awoken by the kiss of a handsome prince.  In 1937, had the word “problematic” then been in use, it wouldn't have been applied to anything in the plot but by the early 2020s, things had changed.  In the pre Trump 2.0 era, when DEI (diversity, equity & inclusion) was compulsory, having Snow White gaining her name because her skin was as “white as snow” and the very existence of dwarfs were both definitely “problematic” so the challenge was to keep the “Snow White” in the title while changing troublesome content as required.  That's been done before and had the 2024 US presidential election elected someone (probably anyone) else, Snow White could have appeared in cinemas to lukewarm reviews but a solid box office based on 7-11 year old girls still impressed at Meghan Markle (Meghan, Duchess of Sussex; b 1981) having proved its not only in fairy tales that princes rescue middle-class girls from dreary lives.  Only Fox News would much have bothered with a condemnation.

Times have changed.  Whether it's Snow White or Sleeping Beauty, for a man (whether or not a prince) to kiss an unresponsive female, it's now usually some sort of assault.  An unresponsive female cannot grant consent.

So for Disney, the timing of events was unfortunate but the earlier race and cultural controversies which swirled around the earlier remakes of Mulan (2020) and The Little Mermaid (2023) should have been a warning.  Most jarring perhaps was the absence of “dwarfs” (in the historic sense of the word).  While Snow White is of course the protagonist, in casting terms there was only one of her and seven of them so the substitution of the heptad with “magical creatures” was always going to attract a critique of its own.  According to the studio, it consulted members of the dwarfism community (the so-called “little people”) “to avoid reinforcing stereotypes” before the re-casting but, given the production was, according to many, replete with cultural, sexist and chauvinist tropes, the cancelled dwarfs received less attention than might have been expected.  With reviewers using phrases like “exhaustingly awful reboot” and “tiresome pseudo-progressive additions”, expectations of success for Snow White have been lowered.  

Friday, February 7, 2025

Zoozve

Zoozve (pronounced zooz-vee or zooz-vay)

The orthodox clipping of 524522 Zoozve (provisional designation 2002 VE68), a temporary quasi-satellite (or quasi-moon and technically an asteroid) of the planet Venus.

2024 (sort of): From an accidental coining by a graphic artist preparing a rendering of a stylized poster of the solar system, the asteroid's provisional designation (2002VE) misread and written as ZOOZVE (the text of the descriptors all in upper case).  Another suggested pronunciation is jeuj-vey (as in zhuzh) but zooz-vee & zooz-vay seem more mnemonic.  Zoozve is a proper noun; the noun plural is zoozves.  Although Zoozve is a unique object, in the solar system, doubtlessly there are many more quasi-moons and zoozve (with an initial lower case) may emerge as the generic term, thus the need for the noun plural.

The Poster.

Zoozve first came to wider public attention early in 2024 when the tale was revealed in a podcast produced by Latif Nasser (b 1986) of New York public radio station WNYC’s RadioLab.  The story was triggered when he first noticed a detail on a poster of the solar system: a moon of Venus called Zoozve.  There are many moons in the solar system but Dr Nasser holds a PhD from Harvard's History of Science department and knew the astronomical orthodoxy was that Venus “has no moons”, something some rapid research confirmed so he contacted Elizabeth Landau (b 1975), a member of the US National Aeronautics and Space Administration's (NASA) communications, his not unreasonable assumption being if anyone should know about what’s in space, it was the folk at NASA.  After consulting the charts, Ms Landau concluded there was such an object but that it wasn’t a moon; it was a quasi-moon which, discovered in 2002, after 2004 when its dual orbits were first tracked, enjoyed the distinction of being the first quasi-moon ever found.  What appeared on the poster as “Zoozve” was the graphic artist’s misreading of “2002VE”, a designation typical of the naming conventions used in astronomy.

Poster close-up.

The distinction between a moon and a quasi moon is the former have “a primary anchor”: Although the Earth’s Moon of course revolves around the Sun as well as this planet, the solar relationship is a by-product of Earth’s gravitational pull.  A quasi-moon is one with two distinct paths of rotation, one around its (temporary) planet and one around the Sun.  There are implications in that beyond the cosmic phenomenon being a scientific curiosity: quasi-moons eventually will become detached (astronomers seem to like “flung-off” which is more illustrative) which means they could become objects which could crash into Earth.  Zoozve is some 240m (785 feet) in diameter and the conventional calculation is an impact with Earth would release energy equivalent to some 69,000 A-bombs with the yield (15 kilotons of TNT) of the device dropped on Hiroshima in 1945.  Zoozve is in the last few hundred years of its eight millennia-odd attachment to Venus and modelling suggests it is unlikely to hit earth when it does become adrift but such calculations are acknowledged to be “ultimately imprecise” and, as mentioned, there are doubtless many more; the universe is a violent and destructive place.  Quasi-moons had been speculated to exist for almost a century before 2002VE was named and since then it’s been discovered Earth has a few of its own.

2002VE was discovered in 2002 by Brian Skiff (b 1953), a research scientist at Arizona’s Lowell Observatory in Arizona and because he made no attempt to give it a “proper” name, it was allocated the procedural 2002VE86 (“proper” names granted usually only after an object has attracted sufficient interest to generate academic papers).  Dr Nasser however was so charmed by the tale of 2002VE that he submitted an application to the Working Group Small Bodies Nomenclature (WGSBN) of the International Astronomical Union (IAU) the committee responsible for assigning names to minor planets and comets.  What he wanted was for 2002VE to become Zoozve but it transpired there were naming "rules" including:

(1) 16 characters or less in length

(2) Preferably one word

(3) Pronounceable (in some language)

(4) Non-offensive

(5) Not too similar to an existing name of a Minor Planet or natural Planetary satellite.

(6) The names of individuals or events principally known for political or military activities are unsuitable until 100 years after the death of the individual or the occurrence of the event.

(7) Names of pet animals are discouraged

(8) Names of a purely or principally commercial nature are not allowed.

(9) Objects that approach or cross Earth's orbit (so called Near Earth Asteroids) are generally given mythological names.

Mar-a-Lago, Palm Beach, Florida.

Because of 2002VE’s proximity to earth, the need to have the name rooted in mythology was obviously the most onerous hurdle to overcome and it is a common-sense stipulation, imposed to avoid controversy on Earth: Imagine the fuss if quasi-moon 524522 Lindsay Lohan ended up crashing into Trump Tower or Mar-a-Lago.  There would be litigation.

Added to which, the IAU have the reputation of being a bunch of humorless cosmic clerks, something like the Vogons ("...not actually evil, but bad-tempered, bureaucratic, officious and callous.") in Douglas Adams’ (1952–2001) Hitchhiker's Guide to the Galaxy (1979-1992): they were the crew who decided Pluto should no longer be thought a planet because of some tiresome technical distinction.  Although lacking the lovely rings of Saturn (a feature shared on a smaller scale by Jupiter, Uranus & Neptune), Pluto is the most charming of all because it’s so far away; desolate, lonely and cold, it's the solar system’s emo.  If for no other reason, it should be a planet in tribute to the scientists who, for decades during the late nineteenth and early twentieth centuries, calculated possible positions and hunted for the elusive orb.  In an example of Donald Rumsfeld's (1932–2021; US secretary of defense 1975-1977 & 2001-2006) “unknown knowns”, the proof was actually obtained as early as 1915 but it wasn’t until 1930 that was realized.  In an indication of just how far away Pluto lies, since the 1840s when equations based on Newtonian mechanics were first used to predict the position of the then “undiscovered” planet, it has yet to complete even one orbit of the Sun, one Plutonian year being 247.68 years long.  Unromantic, the IAU remains unmoved.  Still, there have been exceptions to the rule and it emerged some of the “rules” are actually “guidelines” and the WGSBN was so impressed by the serendipitous tale that a majority of the committee’s eleven voting members cast their ballots for Zoozve so, on 5 February 2024, Radiolab was able to announce the IAU officially had re-designated 2002VE as 524522 Zoozve.

Truly unique words (in the sense of one-off spellings) happen for many reasons.  Those intended for global use as trademarked company or product names really do have to be unique and sufficient different to just about every other word to ensure there are no legal maneuverings contesting their registration which is how we ended up with “Optus” (used since 1991 by the Australian telecommunications company (TelCo) which is now a subsidiary of Singapore-based TelCo Singtel) and Stellantis (a conglomerate created by the merger of the Italian Fiat Chrysler Automobiles (FCA) and the French PSA Group (comprising the Peugeot, Citroën, DS, Opel and Vauxhall brands)).  While on first hearing, to many, Optus and Stellantis probably sounded like mistakes, some words really were just the result of error.  Apron (an article of clothing worn over the front of the torso and at least part of the legs and donned by (1) cooks, butchers and others as protection from spills and (2) Freemasons as part of their regalia worn during their cultish rituals was from the Middle English naperoun & napron, from the Old French napperon, a diminutive of nappe (tablecloth), from the Latin mappa (napkin).  Napron” became “apron” by the process of linguistic assimilation (ie “a napron” becoming “apron” because of the evolution of pronunciation.

Some become legion as accidental coinings only for it to turn out there’s a pedigree.  Warren Harding (1865-1921; US President 1921-1923), during the 1920 presidential campaign, used “normalcy” instead of “normality” after a George W Bush-like (George XLIII, b 1946; US president 2001-2009) mangling of the written text, something understandable because the section with the offending word was almost aggressively alliterative:

America’s present need is not heroics, but healing; not nostrums, but normalcy; not revolution, but restoration; not agitation, but adjustment; not surgery, but serenity; not the dramatic, but the dispassionate; not experiment, but equipoise; not submergence in internationality, but sustainment in triumphant nationality.

In saying "normalcy" he may have misspoken or perhaps Harding liked the word; questioned afterwards he said he found it in a dictionary which probably was true although whether his discovery came before or after the speech wasn't explored.  Although Harding’s choice was much-derided at the time, normalcy had certainly existed since at least 1857, originally as a technical term from geometry meaning the "mathematical condition of being at right angles, state or fact of being normal in geometry" but subsequently it had appeared in print as a synonym of normality on several occasions.  Still, it was hardly in general use though Harding gave it a boost and it’s not since gone extinct, now with little complaint except from the most linguistically fastidious who insist the use in geometry remains the only meaning and all subsequent uses are mistakes.

Sunday, November 17, 2024

Now

Now (pronounced nou)

(1) At the present time or moment (literally a point in time).

(2) Without further delay; immediately; at once; at this time or juncture in some period under consideration or in some course of proceedings described.

(3) As “just now”, a time or moment in the immediate past (historically it existed as the now obsolete “but now” (very recently; not long ago; up to the present).

(4) Under the present or existing circumstances; as matters stand.

(5) Up-to-the-minute; fashionable, encompassing the latest ideas, fads or fashions (the “now look”, the “now generation” etc).

(6) In law, as “now wife”, the wife at the time a will is written (used to prevent any inheritance from being transferred to a person of a future marriage) (archaic).

(7) In phenomenology, a particular instant in time, as perceived at that instant.

Pre 900: From the Middle English now, nou & nu from the Old English (at the present time, at this moment, immediately), from the Proto-West Germanic , from the Proto-Germanic nu, from the primitive Indo-European (now) and cognate with the Old Norse nu, the Dutch nu, the German nun, the Old Frisian nu and the Gothic .  It was the source also of the Sanskrit and Avestan nu, the Old Persian nuram, the Hittite nuwa, the Greek nu & nun, the Latin nunc, the Old Church Slavonic nyne, the Lithuanian and the Old Irish nu-.  The original senses may have been akin to “newly, recently” and it was related to the root of new.  Since Old English it has been often merely emphatic, without any temporal sense (as in the emphatic use of “now then”, though that phrase originally meant “at the present time”, and also (by the early thirteenth century) “at once”.  In the early Middle English it often was written as one word.  The familiar use as a noun (the present time) emerged in the late fourteenth century while the adjective meaning “up to date” is listed by etymologists as a “mid 1960s revival” on the basis the word was used as an adjective with the sense of “current” between the late fourteenth and early nineteenth centuries.  The phrase “now and then” (occasionally; at one time and another) was in use by the mid 1400s, “now or never” having been in use since the early thirteenth century.  “Now” is widely used in idiomatic forms and as a conjunction & interjection.  Now is a noun, adjective & adverb, nowism, nowness & nowist are nouns; the noun plural is nows.

Right here, right now: Acid House remix of Greta Thunberg’s (b 2003) How dare you? speech by Theo Rio.

“Now” is one of the more widely used words in English and is understood to mean “at the present time or moment (literally a point in time)”.  However, it’s often used in a way which means something else: Were one to say “I’ll do it now”, in the narrow technical sense that really means “I’ll do it in the near future”.  Even things which are treated as happening “now” really aren’t such as seeing something.  Because light travels at a finite speed, it takes time for it to bounce from something to one’s eye so just about anything one sees in an exercise in looking back to the past.  Even when reading something on a screen or page one’s brain is processing something from a nanosecond (about one billionth of a second) earlier.  For most purposes, “now” is but a convincing (an convenient) illusion and even though, in certain, special sense, everything in the universe is happening at the same time (now) it’s not something that can ever be experienced because of the implications of relativity.  None of this causes many problems in life but among certain physicists and philosophers, there is a dispute about “now” and there are essentially three factions: (1) that “now” happened only once in the history of the known universe and cannot again exist until the universe ends, (2) that only “now” can exist and (3) that “now” cannot ever exist.

Does now exist? (2013), oil & acrylic on canvas by Fiona Rae (b 1963) on MutualArt.

The notion that “now” can have happened only once in the history of our universe (and according to the cosmological theorists variously there may be many universes (some which used to exist, some extant and some yet to be created) or our universe may now be in one of its many phases, each which will start and end with a unique “now”) is tied up with the nature of time, the mechanism upon which “now” depends not merely for definition but also for existence.  That faction deals with what is essentially an intellectual exercise whereas the other two operate where physics and linguistics intersect.  Within the faction which says "now can never exist" there is a sub-faction which holds that to say “now” cannot exist is a bit of a fudge in that it’s not that “now” never happens but only that it can only every be described as a particular form of “imaginary time”; an address in space-time in the past or future.  The purists however are absolutists and their proposition is tied up in the nature of infinity, something which renders it impossible ever exactly to define “now” because endlessly the decimal point can move so that “now” can only ever be tended towards and never attained.  If pushed, all they will concede is that “now” can be approximated for purposes of description but that’s not good enough: there is no now.

nower than now!: Lindsay Lohan on the cover of i-D magazine No.269, September, 2006.

The “only now can exist” faction find tiresome the proposition that “the moment we identify something as happening now, already it has passed”, making the point that “now” is the constant state of existence and that a mechanism like time exists only a thing of administrative convenience.  The “only now can exist” faction are most associated with the schools of presentism or phenomenology and argue only the present moment (now) is “real” and that any other fragment of time can only be described, the past existing only in memory and the future only as anticipation or imagination; “now” is the sole verifiable reality.  They are interested especially in what they call “change & becoming”, making the point the very notion of change demands a “now”: events happen and things become in the present; without a “now”, change and causality are unintelligible.  The debate between the factions hinges often on differing interpretations of time: whether fundamentally it is subjective or objective, continuous or discrete, dynamic or static.  Linguistically and practically, “now” remains central to the human experience but whether it corresponds to an independent metaphysical reality remains contested.

Unlike philosophers, cosmologists probably don’t much dwell on the nature of “now” because they have the “Andromeda paradox” which is one of the consequences of Albert Einstein’s (1879-1955) theory of special relativity.  What the paradox does is illustrate the way “now” is relative and differs for observers moving at different speeds, the effect increasing as distances increase, such as when the point of reference is the Andromeda galaxy, some 2½ million light years distant from Earth.  Under special relativity, what one observer sees and perceives as “now” on Andromeda will, by another, moving at a different relative speed, will perceive as occurring in the past or future.   This can happen at any distance but, outside of computer simulations or laboratories, the effects of relative simultaneity is noticeable (even for relatively slow speeds) only at distance. 

Seated vis-a-vis (literally "face to face"), Lindsay Lohan (b 1986, right) and her sister Aliana (b 1993, left), enjoying a tête-à-tête (literally, "head to head"), La Conversation bakery "& café, West Hollywood, California, April 2012.  Sadly, La Conversation is now closed.

Among the implications of the Andromeda paradox is that although the sisters would have thought their discussion something in the "here and now", to a cosmologist they are looking at each other as they used to be and hearing what each said some time in the past, every slight movement affecting the extent of this.  Because, in a sense, everything in the universe is happening "at the same time", the pair could have been sitting light years apart and spoke what they spoke "at the same time" but because of the speed at which light and sound travel, it's only at a certain distance a "practical" shared "now" becomes possible.