Greta Thunberg is leading kids and adults from 150 countries in a massive Friday climate strike.
Young people from around the world are leading a massive coordinated strike from school on Friday, September 20, to protest government and business inaction on climate change. It is likely to be one of the largest environmental protests in history.
The Global Climate Strike comes just before countries will gather at the United Nations for the Climate Action Summit on September 23, where countries are supposed to ramp up their ambitions to curb greenhouse gases under the 2015 Paris climate agreement. A second worldwide strike is planned for September 27.
“If you can’t be in the strike, then, of course, you don’t have to,” 16-year-old Swedish climate activist Greta Thunberg, the original school striker who last year began demanding more action from her government on climate change with weekly protests, told Teen Vogue. “But I think if there is one day you should join, this is the day.”
Thunberg has become an increasingly influential figurehead and voice for youth climate angst and activism. Since she no longer flies because of the aviation industry’s high carbon emissions, she was offered the opportunity to travel to the US on a zero-emissions sailboat. This week, she’s been in Washington, DC, speaking before Congress and meeting with US lawmakers, including House Speaker Nancy Pelosi (D-CA), before heading to New York City for the strikes and the summit.
Portrayed in this beautiful image is the spiral galaxy NGC 1448, with a prominent disc of young and very bright stars surrounding its small, shining core. Located about 60 million light-years away from the Sun, this galaxy has recently been a prolific factory of supernovae, the dramatic explosions that mark the death of stars : after a first one observed in this galaxy in 1983, two more have been discovered during the past decade.
Visible as a red dot inside the disc, in the upper right part of the image, is the supernova observed in 2003 (SN 2003hn), whereas another one, detected in 2001 (SN 2001el), can be noticed as a tiny blue dot in the central part of the image, just below the galaxy’s core. If captured at the peak of the explosion, a supernova might be as bright as the whole galaxy that hosts it.
This image was obtained using the FORS instrument mounted on one of the 8.2-metre telescopes of ESO’s Very Large Telescope on top of Cerro Paranal, Chile. It combines exposures taken through three filters (B, V, R) on several occasions, between July 2002 and the end of November 2003. The field of view is 7 arcminutes.
Edwin Joseph Bocage (September 20, 1930 – March 18, 2009), known as Eddie Bo, was an American singer and pianist from New Orleans. Schooled in jazz, he was known for his blues, soul and funk recordings, compositions, productions and arrangements. He debuted on Ace Records in 1955 and released more single records than anyone else in New Orleans other than Fats Domino. Eddie Bo worked and recorded for more than 40 different record labels, including Ace, Apollo Records, Arrow, At Last, Blue-Jay, Bo-Sound, Checker, Chess, Cinderella, Nola, Ric (for which business his carpentry skills were used to build a studio), Scram, Seven B, and Swan. He is described at Allmusic as “a sorely underappreciated veteran of the New Orleans R&B scene.” Eddie Bo grew up in Algiers, Louisiana and in the Ninth Ward of New Orleans. He came from a long line of ship builders with the male members of his family being bricklayers, carpenters and masons by day and musicians by night. Eddie’s mother was a self-taught pianist in the style of friend, Professor Longhair. The Bocage family was involved in the traditional jazz community with cousins Charles, Henry and Peter, who played with Sidney Bechet, contributing to jazz orchestras before World War II.
Eric J. Gale (September 20, 1938 – May 25, 1994) was an American jazz and session guitarist. Born in Brooklyn, New York, Gale began playing guitar at the age of 12. Although he majored in chemistry at Niagara University, Gale was determined to pursue a musical career, and began contributing to accompaniments for such stars as Maxine Brown, the Drifters, and Jesse Belvin. He soon began to attract the attention of King Curtis and Jimmy Smith, who began recommending him for studio work. He became known first as a session musician in the 1960s, eventually appearing on an estimated 500 albums. Among the many artists he recorded with were Mose Allison, Aretha Franklin, Bob James, Paul Simon (Gale plays a supporting role in the 1980 film One-Trick Pony, written by and starring Simon), Lena Horne, Quincy Jones, Bob Marley, Nina Simone, Peter Tosh, Grover Washington, Jr., Herbie Mann, Esther Phillips, Joe Cocker, Carly Simon, Van Morrison, Al Jarreau, Dave Grusin, Lee “Scratch” Perry, Paul Douglas and Billy Joel. He also had played in Aretha Franklin’s stage band.
Keith Moore “Red” Mitchell (September 20, 1927 – November 8, 1992), was an American jazz double-bassist, composer, lyricist, and poet. Mitchell was born on September 20, 1927, in New York City. His younger brother, Whitey Mitchell, also became a jazz bassist.
Mitchell was raised in New Jersey by a father who was an engineer and loved music, and a mother who loved poetry. His first instruments were piano, alto saxophone, and clarinet. Although Cornell University awarded him an engineering scholarship, by 1947 he was in the US Army playing bass. The next year he was in a jazz trio in New York City.
Mitchell performed and/or recorded with Mundell Lowe, Chubby Jackson, Charlie Ventura, Woody Herman, Red Norvo, Gerry Mulligan, and, after joining the West Coast jazz scene in the early 1950s, with André Previn, Shelly Manne, Hampton Hawes, Billie Holiday, Stan Seltzer, Ornette Coleman, and others such as Mahalia Jackson. He also worked as a bassist in the TV and film studios around Los Angeles, occasionally appearing on screen. Mitchell also appeared in documentaries about Tal Farlow and Zoot Sims.
Flamenco Fridays with Sevillanas. Sevillanas (Spanish pronunciation: [seβiˈʝanas]) are a type of folk music and dance of Sevilla and its region. They were derived from the Seguidilla, an old Castilian folk music and dance genre. In the nineteenth century they were influenced by Flamenco. They have a relatively limited musical pattern but are rich in lyrics based on country life, virgins, country towns, neighborhoods, pilgrimage, and love themes. The rhythm of Sevillanas can be interpreted as 3/4, although it is generally 6/8. Each sevillana is composed of 4 or sometimes 7 parts, with each part divided into 3 coplas and with each copla made up of 6 movements. During festivals and shows, it is often the Sevillana dancing visitors to Andalusiamistakenly take as Flamenco, as it is a vivid style, full of turns.
The Ring Nebula (also catalogued as Messier 57, M57 or NGC 6720) is a planetary nebula in the northern constellation of Lyra. Such objects are formed when a shell of ionized gas is expelled into the surrounding interstellar medium by a star at the end of its asymptotic giant branch phase, in the last stages of its evolution before becoming a white dwarf. This nebula was discovered by the French astronomer Charles Messier while searching for comets in late January 1779. Messier’s report of his independent discovery of Comet Bode reached fellow French astronomer Antoine Darquier de Pellepoix two weeks later, who then independently rediscovered the nebula while following the comet. Darquier later reported that it was “…as large as Jupiter and resembles a planet which is fading” (which may have contributed to the use of the “planetary nebula” terminology). It would be entered into Messier’s catalogue as the 57th object. Messier and German-born astronomer William Herschel speculated that the nebula was formed by multiple faint stars that were unresolvable with his telescope.
M57 is 0.787 kpc (2,570 light-years) from Earth. It has a visual magnitude of 8.8v and photographic magnitude of 9.7p. Photographs taken over a period of 50 years show the rate of nebula expansion is roughly 1 arcsecond per century, which corresponds to spectroscopic observations as 20–30 km s−1. M57 is illuminated by a central white dwarf or planetary nebula nucleus (PNN) of 15.75v visual magnitude.