mick laBriola

Louis-Hector Berlioz (11 December 1803 – 8 March 1869) was a French Romantic composer and conductor. His output includes orchestral works such as the Symphonie fantastique and Harold in Italy, choral pieces including the Requiem and L’Enfance du Christ, his three operas Benvenuto Cellini, Les Troyens and Béatrice et Bénédict, and works of hybrid genres such as the “dramatic symphony” Roméo et Juliette and the “dramatic legend” La Damnation de Faust.

The elder son of a provincial physician, Berlioz was expected to follow his father into medicine, and he attended a Parisian medical college before defying his family by taking up music as a profession. His independence of mind and refusal to follow traditional rules and formulas put him at odds with the conservative musical establishment of Paris. He briefly moderated his style sufficiently to win France’s premier music prize – the Prix de Rome – in 1830, but he learned little from the academics of the Paris Conservatoire. Opinion was divided for many years between those who thought him an original genius and those who viewed his music as lacking in form and coherence.

At the age of twenty-four Berlioz fell in love with the Irish Shakespearean actress Harriet Smithson, and he pursued her obsessively until she finally accepted him seven years later. Their marriage was happy at first but eventually foundered. Harriet inspired his first major success, the Symphonie fantastique, in which an idealised depiction of her occurs throughout.

Berlioz completed three operas, the first of which, Benvenuto Cellini, was an outright failure. The second, the epic Les Troyens (The Trojans), was so large in scale that it was never staged in its entirety during his lifetime. His last opera, Béatrice et Bénédict – based on Shakespeare’s comedy Much Ado About Nothing – was a success at its premiere but did not enter the regular operatic repertoire. Meeting only occasional success in France as a composer, Berlioz increasingly turned to conducting, in which he gained an international reputation. He was highly regarded in Germany, Britain and Russia both as a composer and as a conductor. To supplement his earnings he wrote musical journalism throughout much of his career; some of it has been preserved in book form, including his Treatise on Instrumentation (1844), which was influential in the 19th and 20th centuries. Berlioz died in Paris at the age of 65.

Dámaso Pérez Prado (December 11, 1916 – September 14, 1989) was a Cuban bandleader, pianist, composer and arranger who popularized the mambo in the 1950s. His big band adaptation of the danzón-mambo proved to be a worldwide success with hits such as “Mambo No. 5“, earning him the nickname “The King of the Mambo”. In 1955, Prado and his orchestra topped the charts in the US and UK with a mambo cover of Louiguy‘s “Cherry Pink (and Apple Blossom White)“. He frequently made brief appearances in films, primarily of the rumberas genre, and his music was featured in films such as La Dolce Vita.

Pérez Prado began his career as pianist and arranger for the Sonora Matancera, an internationally successful dance music ensemble from his hometown of Matanzas. He later established his own group and made several recordings in Havana in 1946, including “Trompetiana”, a self-penned mambo and one of the first examples arranged for big band. He then moved to Mexico where he developed this particular genre in multiple forms, including bolero-mambo (with María Luisa Landín), guaracha-mambo (with Benny Moré) and two forms of instrumental mambo he created: mambo batiri and mambo kaen. The success of his 1949 recordings landed him a contract with RCA Victor in the US, which led to a prolific career during the 1950s. His number 1 hit “Cherry Pink (and Apple Blossom White)” was followed by other charting singles, such as a cover of “Guaglione” and his own “Patricia“, both released in 1958. Pérez Prado’s popularity in the US began to decline in the 1960s with the advent of other Latin dance rhythms such as pachanga and, later, boogaloo. Despite several innovative albums and a new form of mambo he called “dengue”, Pérez Prado was never able to duplicate his earlier success and returned to Mexico in the 1970s, where he became a naturalized citizen in 1980. He died in Mexico City in 1989. His son, Pérez Jr., continues to direct the Pérez Prado Orchestra in Mexico City to this day.

Today’s NASA/ESA Hubble Space Telescope Picture of the Week features the glorious spiral galaxy NGC 5643, which is located roughly 40 million light-years away in the constellation Lupus. NGC 5643 is what’s known as a grand design spiral, referring to how the galaxy’s two large, winding spiral arms are clear to see. The spiral arms are defined by bright blue stars, lacy reddish-brown dust clouds and pink star-forming regions.

As fascinating as the galaxy appears at visible wavelengths, some of NGC 5643’s most interesting features are invisible to the human eye. Ultraviolet and X-ray images and spectra of NGC 5643 show that the galaxy hosts an active galactic nucleus: an especially bright galactic core powered by a feasting supermassive black hole. When a supermassive black hole ensnares gas from its surroundings, the gas collects in a disc that heats up to hundreds of thousands of degrees. The superheated gas shines brightly across the electromagnetic spectrum, but especially at X-ray wavelengths.

NGC 5643’s active galactic nucleus isn’t the brightest source of X-rays in the galaxy, though. Researchers using ESA’s XMM-Newton discovered an even brighter X-ray-emitting object, called NGC 5643 X-1, on the galaxy’s outskirts. What could be a more powerful source of X-rays than a supermassive black hole? Surprisingly, the answer appears to be a much smaller black hole! While the exact identity of NGC 5643 X-1 is not yet known, evidence points to a black hole that is about 30 times more massive than the Sun. Locked in an orbital dance with a companion star, the black hole ensnares gas from its stellar companion, creating a superheated disc that outshines the galactic centre.

NGC 5643 was also the subject of a previous Picture of the Week. The new image incorporates additional wavelengths of light, including the red color that is characteristic of gas heated by massive young stars.

[Image Description: A close-up of a spiral galaxy, seen face-on. Its center is a bright white point, surrounded by a large yellowish oval with thin lines of dust swirling in it. From the sides of the oval emerge two bright spiral arms which wind through the round disc of the galaxy, filled with shining pink spots where stars are forming and more dark reddish dust. Many stars can be seen in the foreground, over and around the galaxy.]

Once again I have secured the Percussion Chair for this Alien Plant Consuming production of LSOH by Theatre 55. Music supported by Shirley Mier, Lyra Olson, Jamie Carter and mick Bamboula. Along with my stellar vocalists Van Nixon & Patty Lacy. Awesome!

“If a pick pocket meets a Holy Man, he will see only his pockets.” Baba Hari Dass

Sunday 12-8-24 3pm Alto Cumulous Clouds spotted due west from Webber Park in North Minneapolis.

Located in the Centaurus constellation, this gas cloud is part of the giant Running Chicken Nebula. Some people see it as the head of the chicken, others see the chicken’s rear end. But as much as scientists love fun names for nebulae, they are often not very conducive to clear communication in an international field like astronomy. That is why this nebula is formally known by two names that sound, well… a little less funky. In 1955, Australian astronomer Colin Stanley Gum made an inventory of 84 emission nebulae in the southern sky: the Gum catalog. This one is known, quite dryly, as Gum 40. Long before Gum, in 1888, Danish astronomer John Louis Emil Dreyer had already compiled the ambitious New General Catalogue of Nebulae and Clusters of Stars (NGC), an index of 7840 astronomical objects such as galaxies, star clusters and emission nebulae like this one. Dreyer later added two Index Catalogues (IC) to his work, describing another 5386 celestial objects. This nebula was labelled IC 2872. The NGC is still used today: it got its most recent update in 2019, with 13 957 new objects. This image of IC 2872 — or Gum 40, the chicken head or whatever nickname you might wish to give it — was captured by the VLT Survey Telescope (VST), hosted at ESO’s Paranal Observatory in Chile. As telescopes and instruments keep getting better, more and more deep-sky objects are discovered, so the lists and catalogues will never be complete. But that shouldn’t keep us from trying to compile them — or making up fun nicknames, right?