Newmanesque

Newmanesque (pronounced new-min-esk)

The feelings of wonderment, awe, fear and enchantment induced in one when looking to the stars.

1860: From the writings of Cardinal Saint John Henry Newman (1801-1890), the construct being Newman + esque.  The -esque suffix was from the French -esque (-ish, -ic, -esque), from the Italian -esco, from the Latin -iscus, of Germanic origin, from the Lombardic -isc (-ish), from the Proto-West Germanic -isk, from the Proto-Germanic -iskaz (-ish), from the primitive Indo-European -iskos.  It was cognate with the Old High German -isc (from which German gained -isch), the Old English –isċ, the Old Norse –iskr and the Gothic -isks.   It was appended to nouns (particularly proper nouns) to form adjectives in the sense of (1) resembling or tending towards and (2) in the style or manner of.  English picked up the suffix directly as –ish; the -esque suffix technically means a stronger association than -ish or -ite but is often anyway preferred for literary effect.   

Saint John Henry Newman (1801-1890).

John Henry Newman was a poet and theologian, first an evangelical Anglican priest (albeit one gradually assuming a higher ecclesiastical tone) who later, despite having once described the Roman church as "…polytheistic, degrading and idolatrous" became a Roman Catholic cardinal.  This appears to have happened because Newman the younger became haunted by the fourth century words of Saint Augustine of Hippo (354–430), Securus judicat orbis terrarum!, usually translated by scholars as “the verdict of the world is conclusive” and by theologians as “wherefore the entire world judges out of security, they are not good who separate themselves from the entire world, in whatever part of the entire world”.

To structuralists, it means “it is good to keep the sinners in our midst if this is the way we may convert them”.  Newman dwelt on this for some time, an indication it’s not good for impressionable souls to read Augustine at too young an age.  Among the laity, Newman is most remembered for what’s called the newmanesque or the newmanist: the sense of awe wonderment even atheists might feel when gazing at the stars.  In July 2019, Pope Francis (b 1936; pope since 2013) announced at the Consistory of Cardinals that Newman would be created a saint and his canonisation was formally announced on 13 October, thus becoming the first English saint since the seventeenth century.  It’s a long process: Newman was proclaimed "Venerable" by the Congregation for the Causes of Saints in 1991 and was beatified in 2010.  Canonisation was the final step.

The Newmanesque: Look back in awe

Hubble Space Telescope Image NGC 6302 (butterfly nebula), 27 July 2009.

Image NGC 6302, commonly called the butterfly nebula, was taken by the Hubble telescope on 27 July 2009.  Something of a celestial Rorschach test card, cosmic reality belies the delicate appearance of this butterfly, those fragile-looking wings actually boiling cauldrons of gas, swirling at some 36,000^o F (20,000^o C) and travelling through space at 600,000 mph (960,000 km/h), fast enough to travel between earth and the moon in little more than twenty minutes.  The butterfly is in our Milky Way galaxy, some 3800 light-years distant in the constellation of Scorpius, the glowing gas the star’s outer layers, expelled over two millennia, the wingspan more than two light-years across.

At the centre lies a dying star once five times the mass of the Sun but, with its envelope of gases ejected, it’s now unleashing the stream of ultraviolet radiation that gives the cast-off material its glow.  The central star can’t be seen because of the surrounding thick belt of dust which constricts its outflow, creating the classic “bipolar” or hourglass shape shared with many planetary nebulae.  The data from Hubble do however allow scientists to construct a picture with the surface temperature estimated to be over 400,000^o F (220,000^o C), making it one of the Milky Way’s hotter stars.  Before losing the extended outer layers, the star had evolved into a red giant, with a diameter a thousand times that of the Sun, some of the cast-off gas creating the doughnut-shaped ring while other gas was ejected perpendicular to the ring at higher speeds, producing the butterfly’s elongated wings.  Later, as the star heated, a faster stellar wind (a stream of charged particles), ploughed through the structure, again modifying the shape.