|
|
|
Johannes
Kepler (1571-1631) |
Nicolas Copernicus (1473-1543) |
Giuseppe Piazzi (1746-1826) |
Aristarchus (310–230
BC), a Greek astronomer and mathematician,
designed a method to measure the distances to and sizes
of the Sun and the Moon. Because he deduced that the
Sun was so much bigger than the Moon, he concluded that
the Earth must therefore revolve around the Sun.
Aristotle (384-322
BC), a Greek physician and philosopher, believed
that the universe had never had a beginning and would
never end, that it was eternal. In his treatise Meteorology,
he describes meteors, comets, and the Milky Way as “atmospheric
phenomena.” Although Aristotle's writings were
based on first-hand observation, they were later used
to impede observational science.
Johann Bode (1747-1826)
was a German astronomer of the Academy of Science in
Berlin from 1772 to 1825 and director of the Berlin
Observatory from 1786. His most noted contribution to
astronomy is the Uranographia (1801), a collection
of star maps and a catalog of 17,240 stars and nebulae.
In 1772, he devised a formula to express the relative
distances of the Solar System planets from the Sun.
This formula sometimes referred to as Titius' Law, the
Titius-Bode Law, or Bode's Law.
Tycho Brahe, (1546-1601),
a Danish astronomer working in Germany, made a remarkable
star catalogue of over 1000 stars based on his significant
improvements of methods and accuracy in observations.
His wall quadrant and other instruments were widely
copied and led to improved stellar instruments. Kepler
used Tycho Brahe's observations when he constructed
his famous laws of planetary movement.
Nicolas Copernicus (1473-1543) was
born Mikolaj Kopernik. This Polish amateur astronomer
and clergyman is said to be the founder of modern astronomy.
After studying astronomy at the University of Kraków,
he spent a number of years in Italy studying various
subjects, including medicine and canon law. Sometime
around 1500, he lectured in Rome on mathematics and
astronomy. In 1512, he settled in Frauenburg, East Prussia,
where he had been nominated canon of the cathedral.
There he performed his canonical duties and also practiced
medicine. In 1530, Copernicus completed and gave to
the world his great work De Revolutionibus Orbium
Coelestium, which asserted that the Earth rotated
on its axis once daily and traveled around the Sun once
yearly. That treatise was not published until 1543,
when Copernicus was on his deathbed. His beliefs concerning
the universe came to be known as the Copernican system.
Louis Jacques Mandé
Daguerre (1787-1851), French painter and physicist,
invented the daguerreotype in 1839, which was the first
practical process of photography using silver on a copper
plate.
Galileo Galilei (1564-1642),
a scientist, author, and astronomer, discovered the
satellites of Jupiter, the rings of Saturn, the changing
shape of Venus, sunspots and solar rotation. His Juvenilia,
dating from 1584, was mostly paraphrases of Aristotelian
physics and cosmology. Galileo's rising reputation as
a mathematician and natural philosopher (physicist)
gained him a teaching post at the University of Pisa
in 1589 and in 1592 at the University of Padua in the
Venetian Republic. In 1604, Galileo publicly declared
that he was a Copernican. Galileo succeeded in making
a workable and sufficiently powerful telescope with
a magnifying power of about 40. He turned the telescope
toward the sky sometime in the fall of 1609, and within
a few months, he gathered astonishing evidence about
mountains on the Moon, about moons circling Jupiter,
and about an incredibly large number of stars, especially
in the belt of the Milky Way.
Annibale de Gasparis
(1819 –1892) was an Italian astronomer.
His first asteroid discovery was 10 Hygeia in 1849.
Between 1850 and 1865, he discovered eight more asteroids.
From 1864–1889, he was the director of the Capo
di Monte Observatory in Naples. He won the Gold Medal
of the Royal Astronomical Society in 1851. The lunar
crater de Gasparis with a 30-kilometer diameter is named
in his honor, as well as the Rimae de Gasparis, a 93-kilometer
long fracture near the crater, and asteroid 4279.
Carl Friedrich Gauss (1777-1855) was
a German mathematician, a giant among mathematical giants.
As a young man, he made fundamental contributions to
number theory, for which he invented the theory of congruences,
a basic tool to this day. His theorems on line and surface
integrals lie at the heart of modern physics and are
essential for understanding electromagnetism. Gauss
was one of the discoverers of non-Euclidean geometry.
He conducted experiments to determine whether space
was flat, negatively curved, or positively curved by
accurately surveying a large triangle with vertices
at three mountain tops, then seeing whether the sum
of the interior angles is equal to zero, less than zero,
or greater than zero. He found space to be flat, within
the limits of experimental error. Gauss developed many
computational tools and applied them to computing the
orbits of planets and moons.
Tom Gehrels (1925- ),
Dutch-American astronomer, was involved in the Palomar-Leiden
Survey, observing smaller areas of the sky and making
brightness and distance measurements of some 1,800 asteroids.
In 1971, Gehrels edited the first text on asteroids
and organized the first asteroid conference in Tucson,
Arizona. He was the founder and General Editor of the
Space Science Series of the University of Arizona Press.
He helped to set up Spacewatch, a project at the University
of Arizona that specializes in the study of minor planets,
including various types of asteroids and comets. Dr.
Gehrels and his colleagues observe with the 0.9-meter
and 1.8- meter Spacewatch telescopes on Kitt Peak, which
detect mostly main belt asteroids but also near-Earth
asteroids. Spacewatch discovered a moon of Jupiter,
now named Callirrhoe, which was originally mistaken
for an asteroid, and recovered 719 Albert (a long-lost
asteroid).
Hermann Goldschmidt
(1802-1866), was a German painter and amateur
astronomer who lived and worked above the Café
Procope in Paris, France. He discovered 48 Doris and
49 Pales on the same night, September 17, 1857. By May
5, 1861, he had identified 14 new asteroids. He won
the Gold Medal of the Royal Astronomical Society in
1861. A crater on the Moon is named after him as well
as asteroid 1614 Goldschmidt.
Andrew Graham (1815-1907),
professional astronomer and assistant to Edward Cooper
at Markree Castle Observatory in Ireland, discovered
9 Metis on the night of April 25, 1848. He used a 4-inch
(10-cm) Comet Seeker and an observing plan laid out
by Cooper. It is said that Cooper was too busy to observe
that evening, and on the asteroid’s discovery,
delegated to Graham the choice of a name. Metis was
the only asteroid found from an Irish observatory. Andrew
Graham was born in 1815 in County Fermanagh, Northern
Ireland. He was trained to the use of a meridian circle
at Armagh Observatory, although there is no record of
him being on the staff. He resigned his post at Markree
in 1860 but continued his research at Cambridge Observatory
until his retirement in 1905. He died at Cambridge in
1907.
David Gregory (1659-1708)
started his university studies at the age of 12 at Marischal
College, part of the University of Aberdeen. At the
age of 24, he was appointed professor of mathematics
at the University of Edinburgh, where he taught Newtonian
theories. He was the first university teacher to teach
the 'modern' theories at a time when even Cambridge
was still teaching Greek natural philosophy. In 1690,
there was political and religious unrest in Scotland,
and David decided to leave for England. In 1691, David
was elected Savilian Professor at Oxford. Newton was
a major influence in his appointment. In the same year
he became Savilian Professor, he was elected to be a
Fellow of the Royal Society. In 1702, he published Astronomiae
Physicae et Geometricae Elementa, which was a popular
account of Newton's theories. He also worked on optics
publishing Catoptricae et Dioptricae Sphericae Elementa
in 1695. This work describes telescopes, a special interest
of his. He also experimented with making an achromatic
telescope.
Karl Ludwig Harding (1764-1834)
was a German astronomer, notable for having discovered
the asteroid 3 Juno on September 1, 1804. He was hired
in 1796 by Johann Shröeter as a tutor for his son.
It was in Shröeter’s observatory that he
discovered Juno. He then went to Göttingen to assist
Carl Friedrich Gauss. A crater on the Moon is named
after him and so is the asteroid 2003 Harding.
Karl Hencke (1793-1866)
was a postmaster and amateur astronomer in Driesen,
Prussia. He discovered 5 Astraea and 6 Hebe in 1845.
Hencke was looking for 4 Vesta when he found Astraea.
The King of Prussia awarded him with an annual pension
of $300 for the discovery. Since no asteroids had been
discovered after Vesta, other astronomers had abandoned
their searches for more asteroids, convinced that there
were only four. Hencke began searching in 1830 and was
successful fifteen years later.
Paul Herget (1908-1981)
was Director of The Minor Planet Center at Cincinnati,
Ohio, which was established as the International Astronomical
Union Center for asteroid research in 1947.
Sir William Herschel
(1738-1822) was born in Germany but lived most
of his life in England. By 1773, Herschel had built
a reflecting telescope with a focal length of 5.5 ft.
In his search for double stars, he discovered that one
star actually orbited around the other, the first tangible
proof that gravity extended to stars. Out of this work
came a first in its field, the Catalogue of Double
Stars. In 1781, he discovered a new planet in the
constellation of Gemini, the planet Uranus. One of Herschel's
important discoveries was that the Sun is moving in
space relative to its stellar neighbors. In an attempt
to determine the structure of the Milky Way system,
he used a technique called "star gauging."
During a period 20 years ending in 1802, he had counted
over 90,000 stars in 2400 sample areas.
John Russell Hind (1823-1895)
was a British professional astronomer who began his
career at the Royal Greenwich Observatory. As director
of George Bishop’s private observatory, “South
Villa” at Regents Park in London, England, he
discovered 7 Iris and 8 Flora in 1847. From 1853 to
1891, he was Superintendent of the Nautical Almanac.
Edwin Powell Hubble (1889-1953),
an American astronomer, was a pioneer in the study of
extragalactic astronomy. In 1925, he devised a classification
scheme for the structure of galaxies that is still in
use today and provided the conclusive observational
evidence for the expansion of the universe. Hubble obtained
a law degree at Oxford and briefly practiced law before
earning his Ph.D. in astronomy at Chicago in 1917. After
World War I, Hubble went to Mount Wilson Observatory,
where in 1923 he demonstrated that the Andromeda nebula
was far outside our galaxy and established the island
universe theory, which states that galaxies exist outside
our own. In 1929 Hubble's study of the distribution
of galaxies resulted in the discovery of Hubble's Law,
from which the fundamental cosmological quantity is
derived.
Johannes Kepler (1571-1631),
astronomer and mathematician, studied at Tübingen
and became a professor of mathematics at the Protestant
seminary in Graz in 1594. Sometime during 1596, he started
a correspondence with Tycho Brahe, who was then in Prague.
In 1597, Kepler published his first important work,
Misterium Cosmographicum (“The Cosmographic
Mystery”). It contained his mathematical model
designed to explain the relative distances of the planets
from the Sun in the Copernican system. He announced
his first and second laws of planetary motion in his
1609 publication Astronomia Nova (New Astronomy), which
formed the groundwork of Isaac Newton's discoveries.
It was in this publication that he predicted that there
should be a planet between Mars and Jupiter. His third
law was promulgated in Harmonice Mundi (1619,
Harmony of the World). He succeeded Brahe as court astronomer
to Emperor Rudolf II, and in 1628 became astrologer
to Albrecht von Wallenstein at Zagan in Silesia.
Gerard Kuiper (1905-1973),
American astronomer born in the Netherlands, worked
in the McDonald Observatory in Texas. From 1950 to 1952,
he conducted an asteroid survey using a 10-inch telescope
that recorded asteroids down to a magnitude of 16.5
and photographed the entire ecliptic twice. Kuiper is
considered to be the father of modern planetary science
for his wide ranging studies of the Solar System. In
1951, he proposed the existence of a disk-shaped region
of minor planets outside the orbit of Neptune (now called
the Kuiper Belt) as a source for short-period comets—those
making complete orbits around the Sun in less than 200
years. During the 1960s, Kuiper served as chief scientist
for the Ranger lunar-probe program, choosing crash-landing
sites on the Moon. By analyzing Ranger photographs,
he helped to identify sites for the Surveyor and Apollo
programs. A pioneer in the development of infrared astronomy,
he was honored posthumously when the National Aeronautics
and Space Administration (NASA) named its airborne infrared
telescope the Kuiper Airborne Observatory (1975). Kuiper
was the editor of two encyclopedic works, The Solar
System (4 vol., 1953-58) and Stars and Stellar
Systems (9 vol., 1960-68).
Joseph Lalande (1732-1807),
a French astronomer, was sent to Berlin by the French
Academy to determine the Moon's parallax. From 1762,
he was professor of Astronomy in the Collège
de France and later became director of the Paris Observatory.
His chief work is Traité d'astronomie
(1764), and he also produced the most comprehensive
star catalogue of his time (1801).
Hans Lippershey also
spelled Lipperhey (1570 –1619), spectacle-maker
in Holland, was born in Wesel (western Germany) and
settled in Middelburg, the capital of Zeeland in the
southwesternmost province of the Netherlands. New glass-making
techniques were introduced here by Italians in the 1590s,
and perhaps some ideas about combining lenses were abroad
in this glass-making community. Lippershey is believed
to be the first to apply for a patent for his design
of an early telescope in 1608. Although the patent was
eventually denied because it was felt that the device
could not be kept a secret, Lippershey made several
binocular telescopes for the States General and was
paid handsomely for his services. The surviving records
are not sufficient to decide who was the actual inventor
of the telescope, but Lippershey's patent application
is the earliest record of an actually existing telescope.
Theodore Robert Luther
(1822-1900), professional astronomer at the
Municipal Observatory in Düesseldorf, Germany,
discovered 17 Thetis in 1852. By February 20, 1890,
he had discovered 24 asteroids.
Michael Maestlin (1550-1631),
German pastor and mathematician, attended mathematics
and astronomy lectures given by Peter Apian, a professor
of mathematics, while studying at Tuebingen. Enrolled
in a theological course, he served as an assistant to
Professor Apian. In 1580, after serving in a pastorate,
he was appointed professor of mathematics at the University
of Heidelberg. From 1584-1631, he served as professor
of mathematics at the University of Tuebingen. He was
Kepler’s mathematics teacher and later corresponded
with him. He was an amateur astronomer who made most
of his own astronomical instruments.
Jacob Metius (1571-1635)
invented a device for "seeing faraway things as
though nearby." He also applied to the States General
in the Netherlands for a patent on his telescope and
was denied.
Sir Isaac Newton (1643-1727),
one of the most important figures in the history of
science, made significant contributions in the fields
of physics, astronomy, and mathematics. In his Principia
(1687), considered by many the greatest work of modern
science, he explained the laws of motion and universal
gravitation. Newton's discoveries in optics were presented
in his Opticks (1704), in which he elaborated
his theory that light is composed of corpuscles, or
particles. These discoveries led Newton to the logical
but erroneous conclusion that telescopes using refracting
lenses could never overcome the distortions of chromatic
dispersion. He, therefore, proposed and constructed
a reflecting telescope in 1668, the first of its kind,
and the prototype of the largest modern optical telescopes.
Heinrich Wilhelm Matthäus
Olbers (1758–1840) was a German astronomer
and physician. In 1797, he originated the first satisfactory
method for calculating the orbits of comets, but despite
the fame it brought him, he remained an amateur astronomer
and became a physician. He continued his research on
comets and discovered several. He was the first to detect
the comet of 1815 (Comet Olbers). He also discovered
two asteroids, Pallas (1802) and Vesta (1807). Considering
their orbits and those of the other asteroids then known,
Olbers concluded that they were fragments of a disrupted
planet that had formerly revolved around the Sun. He
is best remembered for Olbers' paradox: “Why is
the sky dark at night?” Assuming that space was
infinite and filled with stars, he suggested the entire
sky should be as bright as the surface of the Sun. The
question had originally been raised by Kepler. The correct
explanation is that our universe is finite both in time
and place, and the total amount of matter and energy
is far too small to light up the night sky.
Johann Palisa (1848-1925)
was an Austrian astronomer. He was a prolific discoverer
of asteroids. Between 1874 and 1923, Palisa discovered
a total of 122 asteroids—28 of them at the Pola
Marine Observatory and the rest at the Vienna Observatory.
Christian Heinrich Friedrich
Peters (1813-1890), born in Denmark, was a
professional astronomer who studied under Carl Friedrich
Gauss. He went to the United States in 1854, where he
worked at Hamilton College in Clinton, New York. He
was a prolific discoverer of asteroids. He found both
144 Vibilia and 145 Adeona on June 3, 1875. In two decades
of searching, he found a total of 48 asteroids.
Giuseppe Piazzi (1746-1826),
an Italian monk and amateur astronomer, discovered Ceres
on January 1, 1801, from his observatory on the island
of Sicily. He became a Theatine monk, professor of theology
in Rome in 1779, and professor of mathematics at the
Academy of Palermo in 1780. He supervised construction
of a government observatory, which opened in 1791 at
Palermo, and was its first director. In 1817, he also
established a government observatory at Naples. In 1803,
he published a catalog of the fixed stars, and in 1814,
he enlarged it to include 7,646 stars. He wrote Lezioni
Elementari di Astronomia in 1817.
Claudius Ptolemaeus (also
known as Ptolemy) (c.87-c.165AD) was a celebrated
Greco-Egyptian mathematician, astronomer, and geographer.
He made his observations in Alexandria and was the last
great astronomer of ancient times. Although he discovered
the irregularity in the Moon's motion and made original
observations regarding the motions of the planets, his
place in the history of science is that of collator
and expounder. He systematized and recorded the data
and doctrines that were known to Alexandrian men of
science. His works on astronomy and geography were the
standard textbooks until the teachings of Copernicus
came to be accepted. The Ptolemaic system represented
the Earth (a globe in form) as stationary in the center
of the universe, with Sun, Moon, and stars revolving
about it in circular orbits and at a uniform rate. From
the center outward the elements were earth, water, air,
fire, and ether. Beyond lay zones or heavens, each an
immense sphere. The planets were assumed to revolve
in small circles, called epicycles, whose centers revolved
around the Earth in the vast circles or deferents of
the spheres. To account for the precession of the equinoxes
and other phenomena, later astronomers found it necessary
to add more epicycles and to make both epicycles and
deferents eccentric.
Pythagoras (c.582–c.507
BC), was a pre-Socratic Greek philosopher and
founder of the Pythagorean school. He migrated from
his native Samos to Crotona and established a secret
religious society or order similar to, and possibly
influenced by, the earlier Orphic cult. We know little
of his life and nothing of his writings. Since his disciples
came to worship him as a demigod and to attribute all
the doctrines of their order to its founder, it is virtually
impossible to distinguish his teachings from those of
his followers. The Pythagoreans were influential mathematicians
and geometricians, and the theorem that bears their
name is witness to their influence on the initial part
of Euclidian geometry. They made important contributions
to medicine and astronomy and were among the first to
teach that the Earth was a spherical planet, revolving
about a fixed point.
George Rheticus (1514-1574),
a German mathematics professor, was born Georg Joachim
von Lauchen Rheticus. He studied mathematics at Zürich.
At 25 years of age, he read one of the Copernicus papers
and sought to study under him. Intending to spend a
few weeks with Copernicus, Rheticus ended up staying
as a house guest for two years, He became Copernicus's
only student and spokesman. He published a popularization
of Copernicus's theories entitled Narratio Prima
in 1540. He also managed to convince Copernicus shortly
before his death to allow publication of De Revolutionibus
Orbium Coelestium. Unfortunately, he left publication
in the hands of Lutheran minister Andreas Osiander,
who did not believe that Copernicus's theory represented
a physical model. He added an unauthorized preface stating
that the contents were merely a device to simplify calculations.
Eugene M. Shoemaker
(1928-1997) was a geologist who influenced
decades of research on the role of asteroids. It was
shortly after 1969, when he arrived at California Institute
of Technology in Pasadena, that he became interested
in extending his geological knowledge of the formation
and distribution of terrestrial and lunar impact craters
to the study of the astronomical objects that formed
them. With Eleanor Helin, he developed a plan to search
for the Apollo asteroids with the 0.46-m Schmidt telescope
at Palomar. This search program had its first success
in July 1973 and was soon, with the help of a number
of students and of collaborations using other Schmidt
telescopes, significantly augmenting the rather meager
knowledge that had been accrued on these objects during
the previous four decades. By the time the observing
program ended, in late 1994, it had produced 40 of the
now 417 known Amor, Apollo, and Aten asteroids (the
orbits of this last group being smaller than that of
the earth).
Johan
Schröeter (1745-1815), a German astronomer
with a private observatory at Lilienthal, Germany, was
elected president of the Societas Lilientalica. In 1777,
he was appointed Secretary of the Royal Chamber of George
III in Hanover, where he met two of William Herschel’s
brothers. Herschel’s discovery of Uranus inspired
Schroeter to pursue astronomy more seriously, and he
resigned his post and became Chief Magistrate of Lilienthal.
He acquired two telescopes made by Herschel and concentrated
almost entirely on observations of the Moon.
Johann Daniel Titius (1729-1696)
was a German astronomer and professor at Wittenberg.
He is best known for formulating the Titius-Bode Law,
which is the observation that orbits of planets in the
Solar System closely follow a simple geometric rule.
It was discovered in 1766 and “published”
(without attribution) in 1772 by Johan Elert Bode. Some
say, however, that Christian Wolff first proposed it
in 1724. The asteroid 1998 Titius is named in his honor.
James Watson (1838-1880),
a Canadian-American astronomer, was the director of
the University of Michigan Detroit Observatory in Ann
Arbor, Michigan from 1863-1879. He wrote the textbook
Theoretical Astronomy in 1868. He discovered
22 asteroids, including the 100th asteroid in 1868.
One of his asteroid discoveries, 139 Juewa, was made
in Beijing in 1874 when Watson was there to observe
the transit of Venus.
Max Wolf (1863-1932)
was a German astronomer and a pioneer of astrophotography.
He worked in Heidelberg, where he discovered more the
200 asteroids, beginning with 323 Brucia in 1891. His
astrophotographic techniques automated the discovery
of asteroids, which sharply increased discovery rates
over the older visual methods. In time-exposure photographs,
asteroids appear as short streaks due to the planetary
motion with respect to fixed stars.
Baron Francis Xaver von
Zach (1754-1832), astronomer and geodesist,
was born in Pest. He was patronized by Duke Ernst of
Saxe-Gotha-Altenburg and built an observatory on the
Seeberg near Gotha. He directed the observatory—one
of the most important of the time—from 1791, when
it was completed, until 1806. During this period, Zach
enlisted 24 astronomers throughout Europe in making
a systematic search for asteroids. They came to be called
the Celestial Police. He also published the Monthly
Correspondene.
|