Relative

Weights

4

Styles

8

Available

Variable

Also Available

Mono

Stylistic Sets

7 Apposite Accrual

↑ Relative Book

Correlating Consistencies

↑ Relative Medium

Supplemented Sizes

↑ Relative Bold

Extending Expanse

↑ Relative Black

Decreasing Dimensions

↑ Relative Italic

Incremental Increase

↑ Relative Medium Italic

Relevant Ranges

↑ Relative Bold Italic

Determined Diameters

↑ Relative Black Italic

General Relativity

The first measurement of this relativistic effect was made by British astronomers in 1919. They used the fact that light deflection changes astronomical observations. The “location of a star in the night sky” is simply short-hand for “the direction from which that star’s light reaches us”.

Lights All
Askew In The
Heavens

Michelson—Morley, 1887
Ives—Stilwell, 1938-1941
Kennedy—Thorndike, 1932
Poincaré–Einstein, 1905

Stars Not Where They Seemed or Were Calculated to be, but Nobody Need Worry. No More in All the World Could Comprehend It, Said Einsteln When His Daring Publishers Accepted It.

Men of Science

Agog Over Results

R R R R
S S S S

Eclipse

Total

when the dark silhouette of the Moon completely obscures the intensely bright light of the Sun.

when the Sun and Moon are exactly in line with the Earth but the Moon is smaller than the Sun

Annular

Hybrid

(aka annular/total eclipse)

shifts between a total and

annular eclipse

Total

Annular

Hybrid

Relativtheorie

The theory of relativity usually encompasses two interrelated theories by Albert Einstein: special relativity and general relativity, proposed and published in 1905 and 1915, respectively.