mick laBriola

Richard Edwin Morrissey (9 May 1940 – 8 November 2000) was a British jazz musician and composer. He played the tenor sax, soprano sax and flute.

Dick Morrissey emerged in the early 1960s in the wake of Tubby Hayes, Britain’s pre-eminent sax player at the time. Self-taught, he started playing clarinet in his school band, The Delta City Jazzmen, at the age of sixteen with fellow pupils Robin Mayhew (trumpet), Eric Archer (trombone), Steve Pennells (banjo), Glyn Greenfield (drums), and young brother Chris on tea-chest bass. He then joined the Original Climax Jazz Band. Going on to join trumpeter Gus Galbraith‘s Septet, where alto-sax player Peter King introduced him to Charlie Parker‘s recordings, he began specialising on tenor saxophone shortly after.

Francisco Hernández Mora, better known as Pancho Quinto, was born on April 23, 1933. He was a Cuban rumba percussionist, teacher and founder of Yoruba Andabo.

Heavyweight Dub Champion

https://www.youtube.com/watch?v=c4XHAZ9hPcs

A new infrared image from ESO’s VISTA survey telescope reveals an extraordinary landscape of glowing tendrils of gas, dark clouds and young stars within the constellation of Monoceros (the Unicorn). This star-forming region, known as Monoceros R2, is embedded within a huge dark cloud. The region is almost completely obscured by interstellar dust when viewed in visible light, but is spectacular in the infrared.

An active stellar nursery lies hidden inside a massive dark cloud rich in molecules and dust in the constellation of Monoceros. Although it appears close in the sky to the more familiar Orion Nebula it is actually almost twice as far from Earth, at a distance of about 2700 light-years. In visible light a grouping of massive hot stars creates a beautiful collection of reflection nebulae where the bluish starlight is scattered from parts of the dark, foggy outer layers of the molecular cloud. However, most of the new-born massive stars remain hidden as the thick interstellar dust strongly absorbs their ultraviolet and visible light.

In this gorgeous infrared image taken from ESO’s Paranal Observatory in northern Chile, the Visible and Infrared Survey Telescope for Astronomy penetrates the dark curtain of cosmic dust and reveals in astonishing detail the folds, loops and filaments sculpted from the dusty interstellar matter by intense particle winds and the radiation emitted by hot young stars.

Keith Jarrett (born May 8, 1945) is an American jazz and classical music pianist.

Jarrett started his career with Art Blakey, moving on to play with Charles Lloyd and Miles Davis. Since the early 1970s he has enjoyed a great deal of success as a group leader and a solo performer in jazz, jazz fusion, and classical music. His improvisations draw from the traditions of jazz and other genres, especially Western classical music, gospel, blues, and ethnic folk music.

In 2003, Jarrett received the Polar Music Prize, the first (and to this day only) recipient of both the contemporary and classical musician prizes,and in 2004 he received the Léonie Sonning Music Prize. His album The Köln Concert (1975) became the best-selling piano recording in history.

In 2008, he was inducted into the Down Beat Hall of Fame in the magazine’s 73rd Annual Readers’ Poll.

Keith Jarrett was born on May 8, 1945, in Allentown, Pennsylvania, to a mother of Hungarian descent and a father of either French or Scots-Irishdescent. He grew up in suburban Allentown with significant early exposure to music. Jarrett possesses absolute pitch, and he displayed prodigious musical talents as a young child. He began piano lessons just before his third birthday, and at age five he appeared on a TV talent program hosted by the swing bandleader Paul Whiteman.

Mary Lou Williams (born Mary Elfrieda Scruggs; May 8, 1910 – May 28, 1981) was an American jazz pianist, arranger, and composer. She wrote hundreds of compositions and arrangements and recorded more than one hundred records (in 78, 45, and LP versions).^[1] Williams wrote and arranged for Duke Ellington and Benny Goodman, and she was friend, mentor, and teacher to Thelonious Monk, Charlie Parker, Miles Davis, Tadd Dameron, Bud Powell, and Dizzy Gillespie.

The second of eleven children, Williams was born in Atlanta, Georgia, and grew up in the East Liberty neighborhood of Pittsburgh, Pennsylvania.

https://www.youtube.com/watch?v=hvHJD5X4ezo

Robert Leroy Johnson (May 8, 1911 – August 16, 1938) was an American blues singer-songwriter and musician. His landmark recordings in 1936 and 1937 display a combination of singing, guitar skills, and songwriting talent that has influenced later generations of musicians. Johnson’s shadowy and poorly documented life and death at age 27 have given rise to much legend. One Faustian myth says that he sold his soul to the devil at a local crossroads of Mississippi highways to achieve success. As an itinerant performer who played mostly on street corners, in juke joints, and at Saturday night dances, Johnson had little commercial success or public recognition in his lifetime.

Johnson was born in Hazlehurst, Mississippi, possibly on May 8, 1911, to Julia Major Dodds (born October 1874) and Noah Johnson (born December 1884). Julia was married to Charles Dodds (born February 1865), a relatively prosperous landowner and furniture maker, with whom she had ten children. Charles Dodds had been forced by a lynch mob to leave Hazlehurst following a dispute with white landowners. Julia left Hazlehurst with baby Robert but after two years sent the boy to Memphis to live with her husband, who had changed his name to Charles Spencer.

https://www.youtube.com/watch?v=3UVgH9JqSnQ&index=19&list=PL840CCFF975230F7E

North Korean music includes kinds of both folk and classical, courtly music, including genres like sanjo, pansori, and nongak. Pansori is long vocal and percussive music played by one singer and one drummer.

Dub Explosion

The second of three images of ESO’s GigaGalaxy Zoom project is a new and wonderful 340-million-pixel vista of the central parts of our galactic home, a 34 by 20-degree wide image that provides us with a view as experienced by amateur astronomers around the world. Taken by Stéphane Guisard, an ESO engineer and world-renowned astrophotographer, from Cerro Paranal, home of ESO’s Very Large Telescope, this second image directly benefits from the quality of Paranal’s sky, one of the best on the planet. The image shows the region spanning the sky from the constellation of Sagittarius (the Archer) to Scorpius (the Scorpion). The very colourful Rho Ophiuchi and Antares region features prominently to the right, as well as much darker areas, such as the Pipe and Snake Nebulae. The dusty lane of our Milky Way runs obliquely through the image, dotted with remarkable bright, reddish nebulae, such as the Lagoon and the Trifid Nebulae, as well as NGC 6357 and NGC 6334. This dark lane also hosts the very centre of our Galaxy, where a supermassive black hole is lurking. The image was obtained by observing with a 10-cm Takahashi FSQ106Ed f/3.6 telescope and a SBIG STL CCD camera, using a NJP160 mount. Images were collected through three different filters (B, V and R) and then stitched together. This mosaic was assembled from 52 different sky fields made from about 1200 individual images totalling 200 hours exposure time, with the final image having a size of 24 403 x 13 973 pixels. Note that the final, full resolution image is only available through Stéphane Guisard.

James Lee Ruffin (May 7, 1936 – November 17, 2014) was an American soul singer, and elder brother of David Ruffin of the Temptations. He had several hit records between the 1960s and 1980s, the most successful being the Top 10 hits “What Becomes of the Brokenhearted” and “Hold On (To My Love)“.

Jimmy Ruffin was born in 1936 in Collinsville, Mississippi, to Eli, a sharecropper, and Ophelia Ruffin. He was approaching his fifth birthday when his younger brother David was born. As children, the brothers began singing with a gospel group, the Dixie Nightingales.

In 1961, Jimmy became a singer as part of the Motown stable, mostly on sessions but also recording singles for its subsidiary Miracle label, but was then drafted for national service. After leaving the Army in 1964, he returned to Motown, where he was offered the opportunity to join the Temptations to replace Elbridge Bryant. However, after hearing his brother David, they hired him for the job instead so Jimmy decided to resume his solo career. Ruffin recorded for Motown’s subsidiary Soul label, but with little success.

Arthur Murray Blythe (July 5, 1940 – March 27, 2017) was an American jazz alto saxophonist and composer. He was described by critic Chris Kelsey as displaying “one of the most easily recognizable alto sax sounds in jazz, big and round, with a fast, wide vibrato and an aggressive, precise manner of phrasing” and furthermore as straddling the avant garde and traditionalist jazz, often with bands featuring unusual instrumentation.

Born in Los Angeles, Blythe lived in San Diego, returning to Los Angeles when he was 19 years old. He took up the alto saxophone at the age of nine, playing R&B until his mid-teens when he discovered jazz. In the mid-1960s, Blythe was part of The Underground Musicians and Artists Association (UGMAA), founded by Horace Tapscott, on whose 1969 The Giant Is Awakened he made his recording debut.

After moving to New York in the mid-70s, Blythe worked as a security guard before being offered a place as sideman for Chico Hamilton (1975–77). He subsequently played with Gil Evans‘ Orchestra (1976–78), Lester Bowie (1978), Jack DeJohnette (1979) and McCoy Tyner (also 1979). Blythe’s group – John Hicks, Fred Hopkins and Steve McCall (drummer) – played Carnegie Hall and the Village Vanguard in 1979.

Admiral Amos Easton (May 7, 1905 – June 8, 1968), better known by the stage name Bumble Bee Slim, was an American Piedmont bluessinger and guitarist.

Easton was born in Brunswick, Georgia. Around 1920 he joined the Ringling Brothers circus. He then returned to Georgia and was briefly married before heading north on a freight train to Indianapolis, where he settled in 1928. There he met and was influenced by the pianist Leroy Carr and the guitarist Scrapper Blackwell.

By 1931 he had moved to Chicago, where he made his first recordings, as Bumble Bee Slim, for Paramount Records. The following year his song “B&O Blues” was a hit for Vocalion Records, inspiring a number of other railroad blues and eventually becoming a popular folk song. In the next five years he recorded over 150 songs for Decca Records, Bluebird Records and Vocalion,often accompanied by other musicians, including Big Bill Broonzy, Peetie Wheatstraw, Tampa Red, Memphis Minnie, and Washboard Sam.

DakhaBrakha is a Ukrainian folk quartet which combines the musical styles of several ethnic groups. It was a winner of the Sergey Kuryokhin Prize in 2009.

Babylonians

In the Heart of the Beast Puppet and Mask Theatre’s 44th Annual MayDay Parade, Ceremony, and Festival

Sunday May 6th 2018 Minneapolis in Powderhorn Park
with POSITIVE VIBRATIONS 630PM Band Stage.

Featuring Van Nixon, Tim Siefkes, Onesmo Kibira, Mikemann Mcmahon, Todd Matheson, Paul Strickland, Larry McCabe and mick.

Reggae music!

In the Heart of the Beast Puppet and Mask Theatre’s 44th Annual MayDay Parade, Ceremony, and Festival

Sunday May 6th 2018 Minneapolis in Powderhorn Park
With BEAU KOO JACKS performing at 6pm Band Stage.

Featuring Van Nixon, Jamie Carter, Todd Matheson, Paul Strickland, Larry McCabe, Tim Siefkes, Eric Hohn and mick.

New Orleans and Mardi Gras music!

In the Heart of the Beast Puppet and Mask Theatre’s 44th Annual MayDay Parade, Ceremony, and Festival

Sunday May 6th 2018 Minneapolis at 330pm in Powderhorn Park
Love Supreme theme this year with many guest artists and musicians.

mick, Gregg Herriges and Anthony Varghese from 2011.

In the Heart of the Beast Puppet and Mask Theatre’s 44th Annual MayDay Parade, Ceremony, and Festival

Sunday May 6th 2018 Minneapolis
Performing with the Community Band at noon 25th & Bloomington into Powderhorn Park.
Performing Misirlou, Shto Mi E Milo, Night Train, Caravan by Fanfare Ciocarlia and much more.

The Antennae Galaxies (also known as NGC 4038 and 4039) are a pair of distorted colliding spiral galaxies about 70 million light-years away, in the constellation of Corvus (The Crow). This view combines ALMA observations, made in two different wavelength ranges during the observatory’s early testing phase, with visible-light observations from the NASA/ESA Hubble Space Telescope.

The Hubble image is the sharpest view of this object ever taken and serves as the ultimate benchmark in terms of resolution. ALMA observes at much longer wavelengths which makes it much harder to obtain comparably sharp images. However, when the full ALMA array is completed its vision will be up to ten times sharper than Hubble.

Most of the ALMA test observations used to create this image were made using only twelve antennas working together — far fewer than will be used for the first science observations — and much closer together as well. Both of these factors make the new image just a taster of what is to come. As the observatory grows, the sharpness, speed, and quality of its observations will increase dramatically as more antennas become available and the array grows in size. This is nevertheless the best submillimetre-wavelength image ever taken of the Antennae Galaxies and opens a new window on the submillimetre Universe.

While visible light — shown here mainly in blue — reveals the newborn stars in the galaxies, ALMA’s view shows us something that cannot be seen at those wavelengths: the clouds of dense cold gas from which new stars form. The ALMA observations — shown here in red, pink and yellow — were made at specific wavelengths of millimetre and submillimetre light (ALMA bands 3 and 7), tuned to detect carbon monoxide molecules in the otherwise invisible hydrogen clouds, where new stars are forming.

Massive concentrations of gas are found not only in the hearts of the two galaxies but also in the chaotic region where they are colliding. Here, the total amount of gas is billions of times the mass of the Sun — a rich reservoir of material for future generations of stars. Observations like these will be vital in helping us understand how galaxy collisions can trigger the birth of new stars. This is just one example of how ALMA reveals parts of the Universe that cannot be seen with visible-light and infrared telescopes.