mick laBriola

This image of the region surrounding the reflection nebula Messier 78, just to the north of Orion’s belt, shows clouds of cosmic dust threaded through the nebula like a string of pearls. The submillimetre-wavelength observations, made with the Atacama Pathfinder Experiment (APEX) telescope and shown here in orange, use the heat glow of interstellar dust grains to show astronomers where new stars are being formed. They are overlaid on a view of the region in visible light.

Messier 78 or M 78, also known as NGC 2068, is a reflection nebula in the constellation Orion. It was discovered by Pierre Méchain in 1780 and included by Charles Messier in his catalog of comet-like objects that same year.

M78 is the brightest diffuse reflection nebula of a group of nebulae that includes NGC 2064, NGC 2067 and NGC 2071. This group belongs to the Orion B molecular cloud complex and is about 1,350 light-years distant from Earth. M78 is easily found in small telescopes as a hazy patch and involves two stars of 10th and 11th magnitude. These two B-type stars, HD 38563 Aand HD 38563 B, are responsible for making the cloud of dust in M78 visible by reflecting their light.

Stephen Robert Nesta “Raggamuffin” Marley (born April 20, 1972) is a Jamaican-American musician who is the son of Bob Marley and his wife Rita Marley. Stephen is an eight-time Grammy Award winner, three times as a solo artist, twice as a producer of younger brother Damian Marley’s ‘Halfway Tree’ and ‘Welcome to Jamrock’ albums, and a further three times as a member of Ziggy Marley & The Melody Makers.

His 2011 album Revelation Pt. 1 – The Root of Life won the Grammy Award for Best Reggae Album in 2012. The follow-up, Revelation Pt. 2 – The Fruit of Life was released on July 22, 2016.

In his self-produced solo albums Mind Control (2007), Mind Control Acoustic (2008), Revelation Part I: The Root of Life (2011) and Revelation Part II: The Fruit of Life (2016) Stephen has displayed artistic creativity previously associated with American legends such as Stevie Wonder and Prince; where the artiste composes and produces all the songs on his album, and plays a variety of the musical instruments himself.

Ernesto Antonio “Tito” Puente (April 20, 1923 – May 31, 2000)  was an American musician, songwriter and record producer. The son of Ernest and Ercilia Puente, native Puerto Ricansliving in New York City’s Spanish Harlem, Puente is often credited as “The Musical Pope”, “El Rey de los Timbales” (The King of the Timbales) and “The King of Latin Music”. He is best known for dance-oriented mambo and Latin jazz compositions that endured over a 50-year career. He and his music appear in many films such as The Mambo Kings and Fernando Trueba‘s Calle 54. He guest-starred on several television shows, including Sesame Street and The Simpsons two-part episode “Who Shot Mr. Burns?“. His most famous song is “Oye Como Va“.

Tito Puente was born on April 20, 1923, at Harlem Hospital Center in the New York borough of Manhattan. His family moved frequently, but he spent the majority of his childhood in the Spanish Harlem area of the city. Puente’s father was the foreman at a razorblade factory.

Lionel Leo Hampton (April 20, 1908 – August 31, 2002) was an American jazz vibraphonist, pianist, percussionist, and bandleader. Hampton worked with jazz musicians from Teddy Wilson, Benny Goodman, and Buddy Rich to Charlie Parker, Charles Mingus, and Quincy Jones. In 1992, he was inducted into the Alabama Jazz Hall of Fame, and was awarded the National Medal of Arts in 1996. Lionel Hampton was born in 1908 in Louisville, Kentucky, and was raised by his mother. Shortly after he was born, he and his mother moved to her hometown of Birmingham, Alabama. He spent his early childhood in Kenosha, Wisconsin, before he and his family moved to Chicago, Illinois, in 1916. As a youth, Hampton was a member of the Bud Billiken Club, an alternative to the Boy Scouts of America, which was off-limits because of racial segregation. During the 1920s, while still a teenager, Hampton took xylophone lessons from Jimmy Bertrand and began to play drums. Hampton was raised Roman Catholic, and started out playing fife and drum at the Holy Rosary Academy near Chicago.

The Heart and Soul nebulae are seen in this infrared mosaic from NASA’s Wide-field Infrared Survey Explorer, or WISE. The image covers an area of the sky over ten times as wide as the full moon and eight times as high (5.5 x 3.9 degrees) in the constellation Cassiopeia.

Located about 6,000 light-years from Earth, the Heart and Soul nebulae form a vast star-forming complex that makes up part of the Perseus spiral arm of our Milky Way galaxy. The nebula to the right is the Heart, designated IC 1805 and named after its resemblance to a human heart. To the left is the Soul nebula, also known as the Embryo nebula, IC 1848 or W5. The Perseus arm lies further from the center of the Milky Way than the arm that contains our sun. The Heart and Soul nebulae stretch out nearly 580 light-years across, covering a small portion of the diameter of the Milky Way, which is roughly 100,000 light-years across.

The two nebulae are both massive star-making factories, marked by giant bubbles that were blown into surrounding dust by radiation and winds from the stars. WISE’s infrared vision allows it to see into the cooler and dustier crevices of clouds like these, where gas and dust are just beginning to collect into new stars. These stars are less than a few million of years old — youngsters in comparison to stars like the sun, which is nearly 5 billion years old.

Also visible near the bottom of this image are two galaxies, Maffei 1 and Maffei 2. Both galaxies contain billions of stars and, at about 10 million light-years away, are well outside our Milky Way yet relatively close compared to most galaxies. Maffei 1 is the bluish elliptical object and Maffei 2 is the spiral galaxy.

All four infrared detectors aboard WISE were used to make this image. Color is representational: blue and cyan represent infrared light at wavelengths of 3.4 and 4.6 microns, which is dominated by light from stars. Green and red represent light at 12 and 22 microns, which is mostly light from warm dust.

George Bernard “Bernie” Worrell, Jr. (April 19, 1944 – June 24, 2016) was an American keyboardist and composer best known as a founding member of Parliament-Funkadelicand for his work with Talking Heads. He is a member of the Rock and Roll Hall of Fame, inducted in 1997 with fifteen other members of Parliament-Funkadelic. Worrell was described by Jon Pareles of The New York Times as “the kind of sideman who is as influential as some bandleaders.”

Worrell was born in Long Branch, New Jersey, and grew up in Plainfield, New Jersey, where his family moved when he was eight.^[1] A musical prodigy, he began formal piano lessons by age three and wrote a concerto at age eight. He went on to study at the Juilliard School and received a degree from the New England Conservatory of Music in 1967. As a college student, Worrell played with a group called Chubby & The Turnpikes; this ensemble eventually evolved into Tavares.

After meeting George Clinton, leader of a Plainfield-based doo wop group called The Parliaments, Worrell, Clinton, The Parliaments and their backing band, The Funkadelics, moved to Detroit, Michigan; thereafter, both groups became collectively known as Parliament-Funkadelic. During the 1970s the same group of musicians separately recorded under the names Parliament and Funkadelic, (among several others), but toured as P-Funk. Worrell played grand piano, Wurlitzer electric piano, Hohner Clavinet, Hammond B3 organ, ARP String Ensemble and Moog synthesizer, co-wrote, and wrote horn and rhythm arrangements on hit recordings for both groups and other associated bands under the “Parliafunkadelicment Thang” production company, and many of his most notable performances were recorded with Bootsy’s Rubber Band, Parlet, The Brides of Funkenstein and The Horny Horns. Worrell recorded a 1978 solo album, All the Woo in the World, with the musical backing of P-Funk’s members.

Dudley Stuart John Moore, CBE (19 April 1935 – 27 March 2002) was an English actor, comedian, musician and composer.

Moore first came to prominence in the UK as one of the four writer-performers in the comedy revue Beyond the Fringe from 1960, and with one member of that team, Peter Cook, collaborated on the television series Not Only… But Also. The double act worked on other projects until the mid-1970s, by which time Moore had settled in Los Angeles to concentrate on his film acting.

His solo career as a comedy film actor was heightened by the success of hit Hollywood films, particularly Foul Play (1978), 10 (1979) and Arthur (1981). For Arthur, Moore was nominated for the Academy Award for Best Actor and won a Golden Globe Award. He received a second Golden Globe for his performance in Micki & Maude (1984).

Flamenco Fridays with Fandango. The current ^3/₄ pattern of the fandango, its distinctive progression (i–iv–V) lyrics with octosyllabic verses and the use of castanets and guitars are well-documented from the 18th century.

The fandangos grandes (big fandangos) are normally danced by couples, which start out slowly with gradually increasing tempo. Many varieties are derived from this one.

The fandanguillos (little fandangos) are livelier, more festive derivations of fandangos. Some regions of Spain have developed their own style of fandangos, such as Huelva (fandangos de Huelva) and Málaga (fandangos de Málaga, or Verdiales). Northern areas such as the Principality of Asturias, the Basque Country and Castile and León have preserved a more relaxed performance.

Discovered in 1784 by the German–British astronomer William Herschel, NGC 4394 is a barred spiral galaxy situated about 55 million light-years from Earth. The galaxy lies in the constellation of Coma Berenices (Berenice’s Hair) and is considered to be a member of the Virgo Cluster.

NGC 4394 is the archetypal barred spiral galaxy, with bright spiral arms emerging from the ends of a bar that cuts through the galaxy’s central bulge. These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the center of NGC 4394 lies a region of ionized gas known as a low-ionization nuclear emission-line region (LINER). LINERs are active regions that display a characteristic set of emission lines in their spectra— mostly from weakly ionized atoms of oxygen, nitrogen and sulphur.

Although LINER galaxies are relatively common, it’s still unclear where the energy comes from to ionize the gas. In most cases it is thought to be the influence of a black hole at the center of the galaxy, but it could also be the result of a high level of star formation. In the case of NGC 4394, it is likely that gravitational interaction with a nearby neighbor has caused gas to flow into the galaxy’s central region, providing a new reservoir of material to fuel the black hole or to make new stars.

Clyde Austin Stubblefield (April 18, 1943 – February 18, 2017) was an American drummer best known for his work with James Brown. A self-taught musician, he was influenced by the sound of natural rhythms around him. His drum patterns on Brown’s recordings are considered funk standards. He recorded and toured with Brown for six years and settled in Madison, Wisconsin, where he was a staple of the local music scene. Often uncredited, samples of his drum patterns were heavily used in hip hop music. He was the recipient of an honorary doctorate in fine arts.

Born to Frank D. and Vena Stubblefield on April 18, 1943, he grew up in Chattanooga, Tennessee. He was inspired to pursue drumming after seeing drummers for the first time in a parade. As a youngster his sense of rhythm was influenced by the industrial sounds of factories and trains around him. He practiced the rhythm patterns he heard, sometimes playing two rhythms together. Years later he said about his drumming approach, “If I think of something (…) if I can hum it, I can play it.” He played professionally as a teenager and performed in local bands such as Blue Shufflers, Inclines, and Cascades.

Clarence “Gatemouth” Brown (April 18, 1924 – September 10, 2005) was an American musician from Louisiana and Texas known for his work as a blues musician, as well as other styles of music. He spent his career fighting purism by synthesizing old blues, country, jazz, Cajun music and R&B styles. His work also encompasses rock and roll, rock music, folk music, electric blues, and Texas blues.

He was an acclaimed multi-instrumentalist, who played an array of musical instruments, including the guitar, fiddle, mandolin, viola, harmonica and drums. He won a Grammy Award for Best Traditional Blues Album in 1983 for his album, Alright Again!. He is regarded as one of the most influential exponents of blues fiddle and has had enormous influence in American fiddlecircles.

Brown’s two biggest musical influences were Louis Jordan and T-Bone Walker.

Brown was born in Vinton, Louisiana, and raised in Orange, Texas. His professional music career began in 1945, playing drums in San Antonio, Texas.

Eurreal Wilford “Little Brother” Montgomery (April 18, 1906 – September 6, 1985) was an American jazz, boogie-woogie and blues pianist and singer.

Largely self-taught, Montgomery was an important blues pianist with an original style. He was also versatile, working in jazz bands, including larger ensembles that used written arrangements. He did not read music but learned band routines by ear—once through an arrangement and he had it memorized.

Montgomery was born in Kentwood, Louisiana, United States, a sawmill town near the Mississippi border, across Lake Pontchartrain from New Orleans, where he spent much of his childhood. Both his parents were of African-American and Creek Indian ancestry. As a child he looked like his father, Harper Montgomery, and was called Little Brother Harper. The name evolved into Little Brother Montgomery, and the nickname stuck. He started playing piano at the age of 4, and by age 11 he was playing at barrelhouses in Louisiana. His main musical influence was Jelly Roll Morton, who used to visit the Montgomery household.

One of the brightest galaxies in planet Earth’s sky is similar in size to our Milky Way Galaxy: big, beautiful Messier 81. Also known as NGC 3031 or Bode’s galaxy for its 18th century discoverer, this grand spiral can be found toward the northern constellation of Ursa Major, the Great Bear. The detailed telescopic view reveals M81’s bright yellow nucleus, blue spiral arms, pink starforming regions, and sweeping cosmic dust lanes. Some dust lanes actually run through the galactic disk (left of center), contrary to other prominent spiral features though. The errant dust lanes may be the lingering result of a close encounter between M81 and its smaller companion galaxy, M82. Scrutiny of variable stars in M81 has yielded one of the best determined distances for an external galaxy — 11.8 million light-years.