Craters (E)
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|
Feature Name |
Lat
|
Long
|
Diam
|
Origin |
|
Eckert
|
17.3N |
58.3E |
2 |
Wallace John ~ (1902-1971), American
astronomer; a pioneer in the use of computers to tabulate
astronomical data. Director of the U.S. Nautical Almanac
Office during World War II. In this post he introduced
machine methods to compute and print tables and began
publication of the Air Almanac in 1940. Eckert
directed the construction of a number of innovative
computers for performing astronomical calculations,
including the Selective Sequence Electronic Calculator (SSEC,
1949) and the Naval Ordnance Research Calculator (NORC,
1954), which for many years was the most powerful computer
in the world. The accuracy of Eckert's calculations of the
Moon's orbit was so good that in 1965 he was able to
correctly show that there was a concentration of mass near
the lunar surface. In 1967, he produced data which improved
on Brown's theory of the Moon. |
|
Eddington
|
21.3N |
72.2W |
118 |
Sir Arthur Stanley ~ (1882-1944), British
astrophysicist and mathematician; succeeded George Darwin as
Plumian Professor of Astronomy at Cambridge (1913), and
became director of the Cambridge Observatory (1914).
Discovered the mass-luminosity relationship for stars,
calculated the abundance of hydrogen, and produced a theory
to explain the pulsation of Cepheid variable stars. |
|
Edison
|
25.0N |
99.1E |
62 |
Thomas Alva ~ (1847-1931), American
inventor; patented 1,093 inventions, more than any other
single person in U.S. history. Most famous for his
development of the first electric light bulb, he also
devised improvements to the telephone and contributed to the
development of motion pictures and sound recordings. Of all
his inventions, Edison was most proud of the phonograph. |
|
Edith
|
25.8S |
102.3E |
8 |
English female name. |
|
Egede
|
48.7N |
10.6E |
37 |
Hans ~ (1686-1758), Danish missionary and
natural historian, born in Norway; known as "The
Apostle of Greenland" because of his Christian
missionary work there which began in 1721 and continued for
fifteen years. His Det gamle Grřnlands nye perlustration
(1729) contained the first extensive description of
Greenland's people, plant and animal life, language and
culture. |
|
Ehrlich
|
40.9N |
172.4W |
30 |
Paul ~ (1854-1915), German immunologist and
physician; discovered the cure to syphilis and advanced the
field of disease immunity. Awarded the 1908 Nobel Prize in
Physiology or Medicine (along with I.I. Mechnikov) "in
recognition of their work on immunity." |
|
Eichstadt
|
22.6S |
78.3W |
49 |
Lorentz ~ (1596-1660), German mathematician
and astronomer. |
|
Eijkman
|
63.1S |
143.0W |
54 |
Christiaan H. ~ (1858-1930), Dutch physician
and researcher; while investigating the disease beriberi
in Java, his observations of dietary deficiency led to the
discovery of vitamins. Awarded the 1929 Nobel Prize in
Medicine "for his discovery of the antineuritic
vitamin" (along with Sir Frederick Gowland Hopkins). |
|
Eimmart
|
24.0N |
64.8E |
46 |
Georg Christoph ~ (1638-1705), German
artist, cartographer and astronomer; created a lunar atlas,
the Genuina Corporis Lunaris Facies, with many
features misplaced, the outlines of most of the maria in
error, and many prominent craters not appearing at all. |
|
Einstein
|
16.3N |
88.7W |
198 |
Albert ~ (1879-1955), German-American
physicist; published three papers in 1905, each of which had
a profound effect on the development of physics. In one
paper, he proposed the theory of special relativity, which
provides a correct description for particles traveling at
high speeds. Einstein also explained the photoelectric
effect by hypothesizing that light consisted of particles
(called photons ) with energy equal to E=hv. Einstein
also provided an explanation of Brownian motion using
kinetic theory, stating that it was caused by random
collisions of molecules. He derived an equation stating that
a suspension of small particles should arrange itself in an
exponentially decreasing manner from bottom up. Einstein
subsequently developed general relativity, which postulated
that uniform acceleration and a gravitational field were
equivalent, a statement known as the gravitational
equivalence principle. It interpreted gravity as a warping
of space-time. Awarded the 1921 Nobel Prize in Physics
"for his services to Theoretical Physics, and
especially for his discovery of the law of the photoelectric
effect." |
|
Einthoven
|
4.9S |
109.6E |
69 |
Willem ~ (1879-1955), Dutch physiologist,
born in Java; awarded the 1924 Nobel Prize in Medicine
"for his discovery of the mechanism of the
electrocardiogram." |
|
El Greco
|
14.0N |
34.7E |
6 |
Domenikos Theotokopoulos, or ~ (c.
1541-1614), Spanish artist, born in Crete; Mannerist
painter, most famous for his epic religious paintings,
including The Madonna and Child with St. Martina and St.
Agnes. |
|
Elger
|
35.3S |
29.8W |
21 |
Thomas Gwyn ~ (1838-1897), British
astronomer; first director of the Lunar Section of the
British Astronomical Association, which kept up interest in
the Moon after the demise of the Selenographic Society.
Using an 8.5" reflector, Elger made many drawings of
the Moon between 1884 and 1896; his sketchbooks survive, and
are now in the possession of the British Astronomical
Association. His The Moon: A full Description and Map of
its Principal Physical Features (1895) is considered one
of the finest lunar atlases produced in its time. |
|
Ellerman
|
25.3S |
120.1W |
47 |
Ferdinand ~ (1869-1940), American
astronomer, educator and photographer; Hale's first
assistant at Mount Wilson Observatory, Ellerman conducted a
one-man expedition to Hawaii to observe and measure Halley's
Comet (1910). |
|
Ellison
|
55.1N |
107.5W |
36 |
Mervyn A. ~ (1909-1963), Irish astronomer;
director of Dunsink Observatory (1957-1963), which amassed a
data bank of almost 700,000 solar images, recorded in the Dunsink
Observatory Publications. Through his involvement with
the International Geophysical Year (IGY), an international
co-operative scientific project, Dunsink became a world data
center for solar research. |
|
Elmer
|
10.1S |
84.1E |
16 |
Charles W. ~ (1872-1954), American optical
engineer; with Richard S. Perkin (q.v.), he founded the
noted American precision optics firm, Perkin-Elmer. |
|
Elvey
|
8.8N |
100.5W |
74 |
Christian T. ~ (1899-1970), American
geophysicist and astronomer; his studies of auroral
phenomena brought international prominence to science in
Alaska. Director of the Geophysical Institute at the
University of Alaska, Fairbanks (1952-1963), vice president
for research (1961-1963) and special assistant to the
president (1963-1967). |
|
Emden
|
63.3N |
177.3W |
111 |
J. Robert ~ (1862-1940), Swiss
astrophysicist and meteorologist. developed a theory of
expansion and compression of gas spheres and applied it to
stellar structure. |
|
Encke
|
4.6N |
36.6W |
28 |
Johann Franz ~ (1791-1865), German
mathematician and astronomer; famous as the discoverer of
short periodic comets. The first object of this family (2P/Encke)
was named after him; it is one of the few comets not named
after the discoverer, but after the one who calculated the
orbit. |
|
Endymion
|
53.9N |
57.0E |
123 |
Greek god; beloved of Selene (q.v.), Greek
goddess of the Moon. |
|
Engel'gardt
|
5.7N |
159.0W |
43 |
Vasilii Pavlovich ~ (1828-1915), Soviet
physicist and astronomer. |
|
Eötvös,
or Eotvos
|
35.5S |
133.8E |
99 |
Báró vásárosnaményi Eötvös Loránd ,
or Roland von ~ (1848-1919), Hungarian nobleman,
philanthropist and physicist; founder of Eötvös Society
(1891), president of the Hungarian Academy of Sciences
(1889-1905), rector of Budapest University (1891-1892),
minister of education (1894). The Eötvös Loránd
University in Budapest was named in his honor. |
|
Epigenes
|
67.5N |
4.6W |
55 |
~ (?-c. 200 B.C.), Greek astronomer;
developed early theories of comets. |
|
Epimenides
|
40.9S |
30.2W |
27 |
~ the Cretan (?-fl. 596 B.C.), Greek
philosopher, mathematician, poet and author; the Epimenides
Paradox ("All Cretans are liars ... One of their own
poets has said so"), attributed to him, is one of the
earliest forms of mathematical logic. |
|
Eppinger
|
9.4S |
25.7W |
6 |
Hans ~, Jnr. (1879-1946), Czechoslovakian
doctor; served as Josef Stalin's personal physician.
Employed by the Nazis at the Dachau concentration
camp, he conducted experiments upon Jewish and Gypsy
prisoners who were given unaltered sea water and sea water
whose taste was camouflaged as their sole source of fluid,
causing severe physical disturbance or death within six to
twelve days. Eppinger killed himself exactly one month
before he was scheduled to testify in the Nuremberg war
crimes trial. (Designation of crater removed by the
International Astronomical Union in October 2002.) |
|
Eratosthenes
|
14.5N |
11.3W |
58 |
~ of Cyrene (c. 275-195 B.C.), Greek
scholar, astronomer and geographer; first to accurately
estimate the diameter of Earth. For several decades, he
served as the director of the famous library in Alexandria.
Also conceived the "Sieve of Eratosthenes," a
method of identifying prime numbers. |
|
Erro
|
5.7N |
98.5E |
61 |
Luis Enrique ~ (1897-1955), Mexican
astronomer, mathematician, author, journalist and government
official; the discoverer of 20 variable stars, he helped to
found and served as first director of the National
Observatory at Tonantzintla, Mexico. The planetarium at the
Instituto Politécnico Nacional in Mexico City was named in
his honor. |
|
Esclangon
|
21.5N |
42.1E |
15 |
Ernest Benjamin ~ (1876-1954), French
astronomer and mathematician; director of the observatory at
Strasbourg (1918), and professor of astronomy (1919) prior
to becoming director of the Observatory at Paris
(1929-1944), where he also served as professor of astronomy
(1930-1946). In 1933, using an astronomical calculation of
time, he started the "talking clock" telephone
service in Paris, carried out in his role as Director of the
Bureau International de l'Heure (1929-1944). |
|
Esnault-Pelterie
|
47.7N |
141.4W |
790 |
Robert A. C. ~ (1881-1957), French-Swiss
sculptor, pilot, aviation engineer and inventor; the fourth
licensed pilot in France, he made his first flight in the
spring of 1907 at his own Aerodrome Toussus-le-Noble. His
epic work, Astronautics (1930), constituted a
landmark review of the problems and prospects of space
travel. A subsequent edition in 1934 gave considerable
attention to interplanetary travel, including the
applications of nuclear power. |
|
Espin
|
28.1N |
109.1E |
75 |
Rev. Thomas H. E. C. ~ (1858-1934), British
astronomer; author of The Elementary Star Atlas and Catalogue
of Red Stars and a founder of the Liverpool Astronomical
Society. |
|
Euclides
|
7.4S |
29.5W |
11 |
Euclid (?-c. 300 B.C.), Greek mathematician;
famous for his Elements, a presentation in thirteen
books of the geometry and other mathematics known in his
day. The first six books cover elementary plane geometry and
have served since as the basis for most beginning courses on
this subject. The other books of the Elements treat
the theory of numbers and certain problems in arithmetic (on
a geometric basis) and solid geometry, including the five
regular polyhedra, or Platonic solids. The great
contribution of Euclid was his use of a deductive system for
the presentation of mathematics. |
|
Euctemon
|
76.4N |
31.3E |
62 |
~ (fl-fl. 432 B.C.) Greek astronomer;
devised a seasonal calendar consisting of a 19-year cycle
with the help of another astronomer, Meton of Athens (q.v.).
Together they made a series of measurements of the length of
the shadow cast by a gnomon, measuring vernal equinox to
vernal equinox, in order to calculate the length of the
tropical year, settling on a 19-year cycle (the Metonic
cycle). Euctemon and Meton also devised another important
astronomical invention, the parapegma, a stone tablet with
inscriptions above pegs to indicate the correspondence
between the risings of stars with certain dates. |
|
Eudoxus
|
44.3N |
16.3E |
67 |
~ of Cnidus (ca. 400-ca. 347 B.C.) Greek
philosopher, astronomer and mathematician; the first Greek
to make a map of the stars, he accepted Plato's notion of
the rotation of the planets around the Earth on crystalline
spheres, but noticed discrepancies with observations.
However, his postulation was equally flawed and failed to
give a proper mechanical explanation. As a mathematician,
his work on ratios formed the basis for Book V of Euclid's Elements,
and anticipated in a number of ways the notion of algebra,
which is otherwise absent from ancient Greek mathematics. |
|
Euler
|
23.3N |
29.2W |
27 |
Leonhard ~ (1707-1783), Swiss mathematician;
arguably the greatest mathematician of the 18th century, and
one of the most prolific of all time. His publication list
extends to 886 papers and books, and his complete works fill
about 90 volumes. Euler's important contributions were so
numerous that terms like "Euler's formula" or
"Euler's theorem" can mean many different things
depending on context. In mechanics, there are Euler angles
(to specify the orientation of a rigid body); Euler's
theorem (that every rotation has an axis); Euler's equations
for motion of fluids; and the Euler-Lagrange equation (that
comes from calculus of variations). The "Euler's
formula" with which most calculus students are familiar
defines the exponentials of imaginary numbers in terms of
trigonometric functions; however, there is another "Euler's
formula" that gives the values of the Riemann zeta
function at positive even integers in terms of Bernoulli
numbers. |
|
Evans
|
9.5S |
133.5W |
67 |
Sir Arthur John ~ (1851-1941), British
archaeologist; became curator of the Ashmolean Museum at
Oxford in 1884. Largely responsible for the excavations of
the Cretan city of Knossos, capital of the Minoan
civilization, which uncovered the site that is open to
visitors today. Not only did Evans discover these remains,
but he substantially restored and reconstructed them. |
|
Evdokimov
|
34.8N |
153.0W |
50 |
Nikolaj N. ~ (1868-1940), Soviet astronomer. |
|
Evershed
|
35.7N |
159.5W |
66 |
John ~ (1864-1956), British astronomer;
discovered the horizontal motion of gases outward from the
centers of sunspots, a phenomenon called the Evershed effect
(1909). Appointed assistant director of the Kodaikanal and
Madras observatories India in 1906, later becoming director.
On an expedition to Kashmir in 1915, he made the first
measurements supporting Einstein's prediction that the
wavelength of light emitted by a massive body — in this
case, the Sun — should be increased by an amount
proportional to the intensity of the local gravitational
field. Returning to England in 1925, he built his own solar
observatory at Ewhurst. |
|
Ewen
|
7.7N |
121.4E |
3 |
Gaelic male name. |
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