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The quarter phase moon (i.e. half moon) taken from the Mount Lowe Observatory, ca.1920 (CHS-845)

Traveling west to east, the full moon, viewed from Merritt Island, Fla., at 10:35 p.m. EST, moves into the Earth's shadow during a lunar eclipse. Eclipses occur when the Sun, Earth and Moon line up. They are rare because the Moon usually passes above or below the imaginary line connecting Earth and the Sun. The Earth casts a shadow that the Moon can pass through -when it does, it is called a lunar eclipse. They can only occur when the moon is "full." During a total lunar eclipse the Moon takes on a dark red color because it is being lighted slightly by sunlight passing through the Earth's atmosphere and this light has the blue component preferentially scattered out (this is also why the sky appears blue from the surface of the Earth), leaving faint reddish light to illuminate the Moon during the eclipse KSC-00pp0092

Oblique view of lunar farside photographed from orbit looking southwest

Western hemisphere of the Moon taken by Galileo spacecraft

Range : 350,000 miles This image of the western hemisphere of the Moon was taken through a green filter by Galileo at 9:35 am PST. In the center is the Orientale Basin, 600 miles in diameter, formed about 3.8 billion years ago by the impact of an streroid-size body. Orientale's dark center is a small mare. To the right is the lunar near side with the great, dark Oceanus Procellarum above and the small, circular, dark Mare Humorum Below. Maria are broad plains formed mostly over 3 billion years ago as vast bassaltic lava flows. To the left is the lunar far side with fewer maria, but, at lower left, the South-Pole-Aitken basin, about 1200 miles in diameter, which resemble Orientale but is much older and more weathered and battered by cratering. The intervening cratered highlands of both sides, as well as the maria, are dotted with bright, young craters. This image was 'reprojected' so as to center visibility of small features. ARC-1990-A91-2007

CAPE CANAVERAL, Fla. – A view of the super moon in the eastern sky over Kennedy Space Center in Florida. The full moon reached perigee, the closest point to Earth in its elliptical pattern, at 11:34 p.m. It appeared 14 percent larger and 30 percent brighter than other full moons of 2012. Photo credit: NASA/Jim Grossmann KSC-2012-2734

Traveling west to east, the full moon, viewed from Merritt Island, Fla., at 10:18 p.m. EST, begins moving into the Earth's shadow, at the start of a lunar eclipse. Eclipses occur when the Sun, Earth and Moon line up. They are rare because the Moon usually passes above or below the imaginary line connecting Earth and the Sun. The Earth casts a shadow that the Moon can pass through -when it does, it is called a lunar eclipse. They can only occur when the moon is "full." During a total lunar eclipse the Moon takes on a dark red color because it is being lighted slightly by sunlight passing through the Earth's atmosphere and this light has the blue component preferentially scattered out (this is also why the sky appears blue from the surface of the Earth), leaving faint reddish light to illuminate the Moon during the eclipse KSC-00pp0091

Earth observation views of the Moon taken from OV-105 during STS-99

To "shoot" the sun. Capt. Edward T. Pollock (left) and Capt. F.B. Littell, scientists of the U.S. Naval Observatory in Washington, will ha... charge of the expedition to observe the total solar eclipse of ... sun from a giant dirigible, "Los Angeles" on Jnuary, 24th

Passage de l'ombre de la Lune au travers de l'Europe dans l'éclipse de Soleil centrale et annulaire : qui s'observent le 1er avril 1764, depuis le Cap St. Vincent extrémité meridionale de l'Espagne, jusqu'au Cap Wardhus, dans la Mer Glaciale /

description

Summary

Relief shown pictorially.

Watermarked at left end with necklace enclosing pointed cross with attached pendant cross and at right end with indecipherable wording.

Includes embellished title cartouche and 2 circular diagrams of "Phases de l'éclipse telles qu'on les observera à Paris".

Available also through the Library of Congress Web site as a raster image.

LC copy imperfect: Small section of margin missing at lower left corner; fold-lined.

Acquisitions control no.: 2005-157

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Tags

europe maps physical solar eclipses maps french passage ombre lune travers éclipse soleil centrale soleil centrale annulaire observent avril depuis cap cap st vincent extrémité meridionale vincent extrémité meridionale espagne jusqu wardhus cap wardhus mer glaciale 1764 european map early works to 1800 general maps geography and map division lattré jean lattré le pauté dagelet elisabeth claire tardieu map jusqu au cap wardhus mer glaciale ultra high resolution high resolution vintage maps
date_range

Date

01/01/1764
person

Contributors

Le Pauté Dagelet, Madame.
Lattré, Madame.
Lattré, Jean.
Tardieu, Elisabeth Claire, 1731-1773.
create

Source

Library of Congress
link

Link

http://www.loc.gov/
copyright

Copyright info

Public Domain

label_outline Explore Jean Lattre, Meridionale, Solar Eclipses

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europe maps physical solar eclipses maps french passage ombre lune travers éclipse soleil centrale soleil centrale annulaire observent avril depuis cap cap st vincent extrémité meridionale vincent extrémité meridionale espagne jusqu wardhus cap wardhus mer glaciale 1764 european map early works to 1800 general maps geography and map division lattré jean lattré le pauté dagelet elisabeth claire tardieu map jusqu au cap wardhus mer glaciale ultra high resolution high resolution vintage maps