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...Paris* by British Choreographer Anthony Tudor, which turned Greek mythology's trio of goddesses into three aging Parisian filles of dubious joie, vying for the favor of a sleepy potential customer (Tudor). Famed Choreographer Agnes de Mille, who danced the part first in 1938, turned up as Venus in droopy net stockings, ruffled corselet and a blonde wig suggesting Gorgeous George playing Lady Godiva. As Juno, Ballerina Viola Essen conveyed the bored allure of a Minsky stripper at the first morning show. And as Minerva, Ballet Theater Angel Lucia Chase achieved the air of a brave but discouraged workhorse...

Author: /time Magazine | Title: Music: Fun at the Ballet | 5/9/1955 | See Source »

...Repas Frugal, he said: "I didn't know they had this. It's worth a fortune." But what held Picasso's attention longest was a plaster Madonna from his boyhood home. Exclaimed Picasso: "We had this statue in Malaga. Actually, it's a statue of Venus which father bought in the flea market. He painted on the tears, draped the figure in plaster-soaked cloth. Now my niece has made a crown of flowers. Good! Good! She continues the tradition...

Author: /time Magazine | Title: Art: Uncle Pablo | 4/25/1955 | See Source »

Nunc iterum ver et ardor adest; Musae et Venus placido de caelo Cantabrigiam descenderunt; histriones classici foriter vigescunt. Sed quales Musae nobis? Plautinae? Et qualis Venus? Secunda? Immo edepol severae Musae tragoediae quibus tantum borribiles irae et mortes pallidae placent. Et non Venus benigna inter nos incedit sed illa Venus dirissima quae tantummodo incastos ritus saeviter fovet. O collegium Harvardianum, quale exemplum maestissimum ver et Venus tibi protulit! Ubinam gentium sunt Nymphae Gratiaeque decentes? Cur nihil nisi membra disiecta? Nam hac in Senecae fabula Ration Stoica nihil potest, et ubique regnat Furor et Cupido ct Caedesl Phaedra enim cui voluptas...

Author: NO WRITER ATTRIBUTED | Title: De Phaedra Nostra | 4/22/1955 | See Source »

...comparing the photographs of faintly banded Venus with parallel lines drawn around a white globe, Dr. Kuiper decided where the Venusian equator must be. This told him the position of the poles and the axis of rotation that passes through them. The axis, he decided, is inclined about 32° from the plane of the ecliptic in which the planets revolve around the sun. Since the earth's inclination is only about 23½°, the seasonal changes of climate on Venus, due to the changing angle of sunlight, may be considerably more pronounced than they are on earth...

Author: /time Magazine | Title: Science: Venus Observed | 3/21/1955 | See Source »

...whole, Dr. Kuiper concluded, the meteorology of waterless Venus must be rather simple. There are no ocean basins to complicate the circulation of the dusty carbon-dioxide winds. The yellow dust merely drifts along; it does not condense unpredictably and fall as capricious rain to confound meteorologists...

Author: /time Magazine | Title: Science: Venus Observed | 3/21/1955 | See Source »

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