Radiance (film)

Radiance is a 1998 Australian independent film. It is the first feature film by Aboriginal director Rachel Perkins about three indigenous sisters who reunite for their mother's funeral. The film is based on the play written by Louis Nowra.

Cast

Production

Rachel Perkins became aware of the play when she saw Trisha Morton-Thomas perform Mae's beach monologue as a part of the Eora College end of year student showcase. Perkins called Louis Nowra to adapt it into a half hour drama but Nowra suggested they make it as a feature.

Awards

Radiance (book)

Radiance is the first book of The Immortals Series's spin - off called The Riley Bloom Series.

Plot

Riley Bloom crossed the bridge into the afterlife following a car crash - with her parents and her beloved dog, Buttercup. The afterlife is situated in - Here & Now . And it turns out that the afterlife is not just an eternity of leisure. Riley meets The Council where she is assigned a job as a Soul Catcher, with weird but maybe cute boy as her guide whose name is Bodhi. Her first assignment will take her back to earth, to everything she's left behind - where she must find the Radiant Boy, a ten-year-old, long - lost spirit in the haunting castles of England for centuries, who doesn't want to move on.

Reviews

"Riley, who appeared in ghost form to her older sister, Ever, in Noël’s bestselling Evermore, takes center stage in this middle-grade spinoff, first in a lanned series. . . . her wit, attitude, and maturation should have readers gladly following her into the second installment."—Publishers Weekly

Radiance (album)

Radiance is a live solo piano album by American pianist Keith Jarrett which was released on the ECM label in 2006. It was recorded in concert in 2002 on October 27 in Osaka and October 30, in Tokyo.

Reception

The Allmusic review by Thom Jurek awarded the album 4.5 stars stating "His process is immediate, poignant, and utterly engaging throughout and marks a new phase in his solo recordings that will spur great interest in any open-minded listener interested in improvisational music.".

Track listing

River Cam

The River Cam is the main river flowing through Cambridge in eastern England. After leaving Cambridge, it flows north and east into the Great Ouse to the south of Ely at Pope's Corner. The Great Ouse connects the Cam to the North Sea at King's Lynn: The total distance from Cambridge to the sea is about 40 mi (64 km) and is navigable for punts, small boats, and rowing craft. The Great Ouse also connects to England's canal system via the Middle Level Navigations and the River Nene.

Name

The original name of the river was the Granta and (unusually) its present name derives from the city of Cambridge (Old English: Grantebrycge) rather than the other way around: After the city's present name developed in Middle English, the river's name was backformed to match. This was not universally applied, however, and the upper stretch of the river continues to be informally known as the Granta. It has been said that the river is the "Granta" above the Silver Street Bridge (in Cambridge) and the "Cam" below it. The Rhee tributary is also formally known as the Cam, and the Granta has a tributary on its upper stretch also known as the Granta.

Cam (disambiguation)

A cam is a mechanical linkage which translates motion.

Cam or CAM may also refer to:

Businesses and organizations

People

Places

Alpha Camelopardalis

Alpha Camelopardalis (Alpha Cam, α Camelopardalis, α Cam) is a star in the constellation Camelopardalis, with an apparent visual magnitude of 4.3. It is the third brightest star in this not very prominent circumpolar constellation, the first and second brightest stars being β Camelopardalis and CS Camelopardalis, respectively. It is the farthest constellational star, with a distance of 6000 light-years from Earth.

This star has a stellar classification of O9 Ia, with the 'Ia' indicating that it is an O-type luminous supergiant. It is a massive star with 31 times the mass of the Sun and 37 times the Sun's radius. The effective temperature of the outer envelope is 30,000 K; much hotter than the Sun's effective temperature of 5,778 K, giving it the characteristic blue hue of an O-type star. It is emitting 620,000 times the luminosity of the Sun and is a weak X-ray emitter.

This star shows multiple patterns of variability. It may be a non-radial pulsating variable star, which is causing changes in the spectrum being emitted by the photosphere. The absorption lines in the optical spectrum show radial velocity variations, although there is significant uncertainty about the period. Estimates range from a period as low as 0.36 days up to 2.93 days. The stellar wind from this star is not smooth and continuous, but instead shows a behavior indicating clumping at both large and small scales. This star is losing mass rapidly through its stellar wind at a rate of approximately 6.3 × 10⁻⁶solar masses per year, or the equivalent of the mass of the Sun every 160,000 years.