History of Astronomy/Concepts of Earth Flashcards

Help prepare for Dantes Exam

1
Q

In the development of _______________ thought, certain original and imaginative individuals began to make systematic observations of celestial objects to formulate theories and explain their behavior.

A

Astronomical. Ancient observers assumed the Earth was vast, immobile, and the center of the universe. Only when scientific procedures were developed did man’s concept of the universe begin to change.

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2
Q

The _______________ must call upon all his resources of ingenuity and employ more clever devises than the most astute detective to solve the problems of his business.

A

Astronomer. Astronomy is the science of the universe, and the laboratory for this science is afar and untouchable, other than the observations of fallen meteorites.

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3
Q

The first significant development of astronomy as a science took place in ancient _____________.

A

Greece. China, India, Mesopotamia, and Egypt had also made celestial observations, even before the Greeks. But the Greeks were the ones who explored a reservoir of ideas and inspirations, and carried out experiments and observations that contributed to the development of astronomy as a science.

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4
Q

The earliest Greek scientists were the ______________, who lived in what is now Asia Minor.

A

Ionians. The foremost astronomers of the Ionians were Thales and Anaximander. Thales introduced the concept of geometry and surveying. Anaximander may have been the first to speculate on the relative distances of the sun, moon, and planets.

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5
Q

_________________ was originally an Ionian in belief, but later founded a school of thought of his own regarding the shape of the planets.

A

Pythagoras. Pythagoras pictured a series of concentric spheres in which each of the seven moving objects, the planets, the sun and the moon, was carried by a separate sphere from the one that carried the stars, so that the motions of the planets resulted from independent rotations of the different spheres about the Earth.

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6
Q

A member of the Pythagorean school, ______________ was the first to introduce the concept that the Earth is in motion.

A

Philolaus. His concept proved to be erroneous in that he believed that there were two earths and that they each revolved equidistant from a central fire. However, he had set the “moving earth” concept in motion.

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7
Q

One of the most famous of the Greek philosophers was ________________.

A

Aristotle. He wrote encyclopedic treatises on nearly every field of human endeavor during his time. Unfortunately, his expositions in astronomy were less sound than some of his other work. The greatest of the Greek accomplishments in the fields of physics and astronomy came post-Aristotle.

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8
Q

The shape of the _________ in the sky depends simply on how much of its daylight hemisphere is turned to our view.

A

Moon. The phases of the moon and of eclipses are the results of illumination by sunlight. The moon itself is not luminous (it does not emit its own light).

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9
Q

_______________ of Samos was the first astronomer of the Alexandrian school and devised an ingenious method to find the relative distances from the Earth to the sun and moon.

A

Aristarchus. His procedure rests on the three assumptions that the moon goes about the Earth in a perfectly circular orbit, that the moon’s orbital velocity is perfectly uniform, and that the sun is near enough that its rays travel along diverging paths to different parts of the moon’s orbit. Although all three of these assumptions are incorrect, he pioneered a scientific approach that could be used to determine the distances from the Earth to the sun and moon.

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10
Q

Aristarchus also devised an ingenious technique to determine the relative ___________ of the sun, moon, and Earth.

A

Sizes. Although the data obtained and used by him were inaccurate and his results somewhat far from the truth, at least they were better than any available before and the first objective measures of astronomical dimensions based on logical reasoning.

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11
Q

The _________________ hypothesis states that the Earth orbits the sun and the Earth is not the center of the universe.

A

Heliocentric. Aristarchus was the first to profess this belief. This is opposed to the geocentric model of the universe, which states that the Earth is at the center of the universe and all objects revolve around it. Aristotle and Ptolemy were believers in the geocentric model.

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12
Q

The greatest astronomer of ancient times was _________________.

A

Hipparchus. His studies are credited with the development of both plane and spherical trigonometry, highly accurate observations, the use of old observations to determine changes, and the invention of a geometrical representation describing the motions of the sun and moon more precisely than ever before.

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13
Q

Another Greek astronomer, Cladius ______________, compiled a series of thirteen volumes on astronomy known as the Almagest.

A

Ptolemy or Ptolemeus. Most of the Almagest is a compilation of the astronomical achievements of the past, especially Hipparchus. However, it does contain some of his own contributions including the measurement of the distance to the moon by a technique essentially identical to the one used today.

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14
Q

Nicolas _______________ was born in Thorn on the Vistula in Poland. His forte was mathematics.

A

Copernicus. His great contribution to science was a critical reappraisal of the existing theories of cosmology and the development of a new model of the solar system.

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15
Q

Copernicus’s excellence as a mathematician and astronomer gave him the information to determine values for the distances of the various ____________ from the sun.

A

Planets. He lived from 1473 – 1543, yet his calculations (as shown by the table below) compared to modern calculations show how advanced he was in his observations and mathematical genius.

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16
Q

After beginning training for a medical career, ______________ found that he had little interest in the subject and later switched to mathematics.

A

Galileo. His refusal to accept dogmatic statements without proof allowed his mathematic abilities to proliferate. In 1589, he became professor of mathematics and astronomy at the university at Pisa.

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17
Q

Galileo’s greatest contributions were in the field of ______________.

A

Mechanics. Galileo experimented with pendulums, with balls rolling down inclined planes, with light and mirrors, with falling bodies, and many other objects. Galileo showed that if a heavy and light object were dropped together, even from a great height, both would hit the ground at practically the same time.

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18
Q

Galileo has often been called the ___________ of modern astronomy.

A

Father. Galileo probably has been the person most widely recognized as the “father of modern astronomy”, although there are many historians that have given the title to Nicholas Copernicus or Johannes Kepler.

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19
Q

The actual first telescope that attracted much notice was built by the Dutch spectacle maker ______ _____________ in 1608, but was only about three power.

A

Hans Lippershey. Historians generally credit Lippershey with the invention of the telescope, as he was the first to apply for a patent for a design. There is uncertainty about whether others had built telescopes earlier in the past.

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20
Q

Galileo was the first known astronomer to build a telescope for the specific purpose of observing and recording celestial bodies. His telescope was about __________ power.

A

Thirty. Hans Lippershey invented the telescope in 1608, intending it for use as a military device. Having heard of the discovery of Hans Lippershey, it was in 1609 that Galileo constructed a much improved refracting telescope of his own. He is the first person credited with using the telescope for looking at the stars. With the aid of his telescope, he was able to make keen observations that were recorded in his book Message from the Stars.

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21
Q

It was Isaac ____________ who formulated the basic laws of modern mechanics and showed them to be universal throughout the solar system, applying to the motions of the celestial objects as well as to objects on the Earth.

A

Newton. His greatest contributions in the fields of astronomy, mechanics, optics, and mathematics were conceived by the time he had reached the age of 24.

22
Q

Newton is also often credited with developing the next big development in telescopes in 1668 (about sixty years after Galileo’s first telescope), the ______________ telescope.

A

Reflecting. The reflecting telescope (also called a newtonian telescope) uses a curved mirror instead of a lens. Netwon’s development of the use of mirrors instead of lenses opened the door to development of telescopes of millions of times magnification–far beyond what could ever be achieved with a lens.

23
Q

Newton’s entire system is based on three laws of ____________.

A

Motion. These three laws are: 1. In the absence of outside forces, the momentum of a system remains constant. 2. If a force acts upon a body, the body accelerates in the direction of the force, its momentum changing at a rate numerically equal to that force. 3. Forces are always mutual, thus if a force is exerted upon a body, that body reacts with an equal and opposite force upon whatever exerts the force upon it.

24
Q

In 1905, Albert Einstein published a paper in which he outlined his theory of ______________.

A

Relativity. Einstein’s theory was based on two postulates: 1. There is no absolute reference system with which we can measure absolute motions in space. The best we can hope to measure is the relative motion of one object with respect to another. 2. The speed of light, with respect to all observers, is always the same.

25
Q

The equatorial circumference of the Earth is ____________ statute miles.

A

24,900. The Earth is not quite perfectly spherical. Along the Earth’s equator one degree is about 60 nautical miles and a nautical mile is 1.1516 statute miles. The formula for figuring the circumference is 360 (degrees in a circle) x 60 (nautical miles in a degree) x 1.1516 (nautical miles in a statute mile).

26
Q

The study of stresses that build up gradually in the crust of the Earth and cause earthquakes is called ______________.

A

Seismology. Energy is often released by slippages along fissures or faults resulting in earthquakes. Some of these vibrations travel along the surface and others pass directly through the interior of the Earth. Seismology is studied through the use of instruments that pick up vibrations and record the activity.

27
Q

The ______________ increases about one degree Celsius for every one hundred feet you go downward into the crust of the Earth.

A

Temperature. As the core slowly cools, conduction gradually transmits heat from the Earth’s interior out through the crust. Cooling of the hot core occurs at a very slow rate.

28
Q

The chemical composition of the Earth’s atmosphere is mostly _____________.

A

Nitrogen. At the Earth’s surface, the constituent gases are found to be 78 percent nitrogen, 21 percent oxygen, and 1 percent argon, with traces of water, carbon dioxide, and other gases. At lower elevations, variable amounts of dust particles and water droplets are also found suspended in the air.

29
Q

The Earth has a ______________ field similar to that produced by a bar magnet.

A

Magnetic. The magnetic poles of the Earth are located about 1200 miles from its geographical poles: the north magnetic pole is in Northeast Canada. The origin of this magnetic field is unknown, although it may be connected with the Earth’s rotation and possibly with electrical currents in the interior.

30
Q

In 1851, a French physicist named Jean Foucault proved that the Earth rotates through the use of a ______________.

A

Pendulum. Foucault suspended a 200 feet pendulum weighing 60 pounds from the domed ceiling of the Pantheon in Paris. He started the pendulum swinging evenly and the direction of swing of the pendulum was recorded on a ring of sand placed on a table beneath its point of suspension. At the end of each swing, a pointed stylus attached to the bottom cut a notch in the sand. After a few moments, the plane of oscillation of the pendulum was slowly changing with respect to the ring of sand, and hence, with respect to the Earth.

31
Q

The _____________ effect is any apparent deflection in the motion of a body resulting from the Earth’s rotation.

A

Coriolis. Any object moving freely over the surface of the Earth appears to be deflected to the right in the Northern Hemisphere and to the left in the Southern Hemisphere because of the rotation of the Earth beneath it.

32
Q

The Earth’s ____________ is a great circle on the Earth’s surface halfway between the North and South Poles.

A

Equator. A great circle is any circle on the surface of a sphere whose center is at the center of the sphere. The equator is such a circle.

33
Q

There is also a series of imaginary great circles that pass through the North and South Poles called _____________.

A

Meridians. These circles intersect the equator at right angles and can be used to specifiy the east-west location of that place.

34
Q

The ______________ of a place is the number of degrees, minutes, and seconds of arc along the equator between the meridian passing through the place and the one passing through Greenwich, England (the Prime Meridian), the site of the old Royal Observatory.

A

Longitude. The measurement for longitude is either to the east or west of the Greenwich meridian from 0° to 180°

35
Q

The ____________ of a specific location is the number of degrees, minutes, and seconds of arc measured along its meridian starting at the equator.

A

Latitude. Latitudes are measured either to the north or south of the equator from 0° to 90°.

36
Q

In denoting positions of objects in the sky, it is often convenient to make use of the fictitious _____________ sphere, a concept that earlier observers accepted literally.

A

Celestial. The celestial sphere can be thought to be a hollow shell of extremely large radius centered on the observer. Coordinate systems, analogous to latitude and longitude can be devised to designate the positions of objects in the sky.

37
Q

By imagining that the meridian of the observer on the Earth is projected upward and outward until it reaches the celestial sphere, it then becomes the observer’s celestial _________________.

A

Meridian

38
Q

The _____________ is the overhead point along the extension of a line from the center of the Earth up through the observer.

A

Zenith. The zenith is the point on the celestial sphere that’s directly over our heads at any given time. Together with the horizon, the zenith is used to denote the position of objects in the sky.

39
Q

The ____________ is a great circle on the celestial sphere 90° from the zenith.

A

Horizon. The horizon passes through the center of the Earth and is parallel to the sensible horizon of a given position or the plane of such a circle.

40
Q

A system that is relative to the observer for specifying the position of a star is the ______________ coordinate system.

A

Horizontal. The horizontal coordinate system uses measurements relative to the observer’s horizon, therefore two people standing in two different parts of the world will have different measurements for the same star. The system consists of two measurements–the azimuth and the altitude. The azimuth runs from 0° to 360° and tells the observer what direction to look in, while the altitude tells the observer how high to look.

41
Q

The plane in which the Earth revolves is 23.5° different than the plane of the equator and this is called the ____________ of the ecliptic.

A

Obliquity. The ecliptic plane is the imaginary plane defined by the projection of Earth’s orbit (the path the Earth follows around the sun) onto the celestial sphere.

42
Q

The ______________ of the Earth result because the plane in which the Earth revolves does not coincide with the plane of the Earth’s equator.

A

Seasons. The Earth’s axis is tilted from the vertical by 23.5° as it makes its orbit around the sun. The result of this tilt (or obliquity of the ecliptic) is that the Northern Hemisphere is inclined toward the sun in June and away from it in December, thus varying temperatures in the seasons.

43
Q

The measurement of _________ is based on the rotation of the Earth.

A

Time. As the Earth turns, objects in the sky appear to move around us, crossing the meridian each day. Time is determined by the position in the sky, with respect to the local meridian, of some reference object on the celestial sphere. The interval between successive meridian crossings or transits of that object is defined as a day and each day is divided into 24 equal parts called hours.

44
Q

The __________ day is the period of the Earth’s rotation with respect to the sun.

A

Solar. A solar day is one complete rotation of the Earth. There are about 365 days in a year (the time it takes to make one complete revolution around the sun) and 360° in a circle. Therefore, the daily motion of the Earth in its orbit is about one degree.

45
Q

With the development of railroads and the telegraph, it became necessary to establish time _________ for the standardization of time within the nation.

A

Zones. In 1883, the continental United States was divided into four time zones; Eastern Standard Time (EST), Central Standard Time (CST), Mountain Standard Time (MST), and Pacific Standard Time (PST). In 1884, an international conference was held in Washington, D.C. in which 26 nations were represented. At that conference it was agreed to establish a system of 24 international time zones around the world.

46
Q

To take advantage of the maximum amount of sunlight during waking hours, ___________ ____________ time was established during the spring and summer.

A

Daylight Saving. Daylight saving time is simply the local standard or zone time of the place plus one hour. Thus, on a summer evening, when it would ordinarily get dark at about 8:00 p.m. standard time, it does not get dark until 9:00 p.m. daylight saving time. The practice of having a daylight saving time is not universal–it varies from country to country.

47
Q

The natural units of the calendar are the ______, based on the period of rotation of the Earth.

A

Day.

48
Q

The __________ is based on the period of revolution of the moon around the Earth.

A

Month.

49
Q

The _________ is based on the period of revolution of the Earth around the sun.

A

Year. The three units of calendar measure–day, month, year–do not divide evenly into any of the others. The period of revolution of the moon around the Earth is about 27 1/3 days. The period of revolution of the Earth around the sun is 365 days, 6 hours, 9 minutes, and 10 seconds. Those extra 6 hours in our orbit around the sun account for why we have a leap year every four years–to accommodate for the extra day that has accumulated.

50
Q

The _________ is an independent unit probably invented by man, although its length may have been based on the interval between the quarter phases of the moon.

A

Week. The seven days of the week are named for the seven planets including the sun and moon as recognized by the ancients.