4-6 Script
... Start with a (light) daytime view of the sky. If it is the wrong time of year to use the current view/time, change to a summer day. Explain that today you are going to talk about astronomy. Discuss the definition: from Greek words that mean "star law," astronomy is a science that studies things in t ...
... Start with a (light) daytime view of the sky. If it is the wrong time of year to use the current view/time, change to a summer day. Explain that today you are going to talk about astronomy. Discuss the definition: from Greek words that mean "star law," astronomy is a science that studies things in t ...
Galileo Galilei (1564-1642) - Sunshine Coast Centre RASC
... makes penicillin, I just found it, one sometimes finds what one is not looking for” ...
... makes penicillin, I just found it, one sometimes finds what one is not looking for” ...
SEPOF_NGSSOptionalWebinar-K-2_26JUN13-2
... solve the same problem to compare the strengths and weaknesses of how each performs. I-PS4-4. Use tools and materials to design and build a device that uses light or sound to solve the problem of communicating over a distance.* [Clarification Statement: Examples of devices could include a light sour ...
... solve the same problem to compare the strengths and weaknesses of how each performs. I-PS4-4. Use tools and materials to design and build a device that uses light or sound to solve the problem of communicating over a distance.* [Clarification Statement: Examples of devices could include a light sour ...
Seasons
... different on Irth – The “A” answer: Irth would have no circumpolar stars at any location • Expect an exam question where a different model leads to different observations (or vice-versa). Full-credit answers depend on specific observations ...
... different on Irth – The “A” answer: Irth would have no circumpolar stars at any location • Expect an exam question where a different model leads to different observations (or vice-versa). Full-credit answers depend on specific observations ...
Lab 02: Determining the Solar and Sidereal Days
... Similarly, we all know that one day is 24 hours long. Our entire calendar is based on this fact! However, the measurement of the rotation rate of any object must be done with respect to some reference point. When we measure the time it takes for the Earth to complete one full rotation, it turns out ...
... Similarly, we all know that one day is 24 hours long. Our entire calendar is based on this fact! However, the measurement of the rotation rate of any object must be done with respect to some reference point. When we measure the time it takes for the Earth to complete one full rotation, it turns out ...
May - RASC St. John`s Centre
... poison them. The shepherds chased after Icarius and killed him. When Dionysus found out he punished the shepherds by placing a plague upon their land. Icarius was raised to the sky and honored as the constellation Boötes. ...
... poison them. The shepherds chased after Icarius and killed him. When Dionysus found out he punished the shepherds by placing a plague upon their land. Icarius was raised to the sky and honored as the constellation Boötes. ...
Theme 3.1 Astronomy of the Ancients Stonehenge Most people
... a great deal about the history of construction of Stonehenge, which was spread over many phases occupying many centuries. Stonehenge is larger than just the obvious set of stones and began with a large circular moat surrounding the set of so called Aubrey holes named after the investigator, 56 of th ...
... a great deal about the history of construction of Stonehenge, which was spread over many phases occupying many centuries. Stonehenge is larger than just the obvious set of stones and began with a large circular moat surrounding the set of so called Aubrey holes named after the investigator, 56 of th ...
early greek astrophysics: the foundations of modern science and
... many valleys and islands, which allowed, or probably, to state it more correctly, led to the development of many societies, which may also have been completely different in their structure and attitudes, as it is illustrated within the differences between the society of Athens and of Sparta. The div ...
... many valleys and islands, which allowed, or probably, to state it more correctly, led to the development of many societies, which may also have been completely different in their structure and attitudes, as it is illustrated within the differences between the society of Athens and of Sparta. The div ...
Sidereal vs. Synodic Motion
... A mean solar day is 24 hours (the “mean” is there to average over the effect of the analemma). The earth has to rotate more than 360° for the sun to come back to “noon”. ...
... A mean solar day is 24 hours (the “mean” is there to average over the effect of the analemma). The earth has to rotate more than 360° for the sun to come back to “noon”. ...
Assignment 2 - utoledo.edu
... motion of planets like Jupiter? a. the planets were not moving along the ecliptic but all over the celestial sphere b. the planets moved in very elongated ellipses, and their speed in orbit changed radically over the course of a year c. the Sun moved among the planets, and pulled them out of their ...
... motion of planets like Jupiter? a. the planets were not moving along the ecliptic but all over the celestial sphere b. the planets moved in very elongated ellipses, and their speed in orbit changed radically over the course of a year c. the Sun moved among the planets, and pulled them out of their ...
October - Sonoma County Astronomical Society
... possibly reaching Earth or beyond. Because these opposite pressures will happen simultaneously, it is hard to predict exactly what will happen next in our own solar system. The fate of V391 Pegasi provides us some clues, but there are important differences between that star and ours. When the sun tu ...
... possibly reaching Earth or beyond. Because these opposite pressures will happen simultaneously, it is hard to predict exactly what will happen next in our own solar system. The fate of V391 Pegasi provides us some clues, but there are important differences between that star and ours. When the sun tu ...
Telescopic Drawings or Photographs of Celestial
... GCSE Astronomy Controlled Assessment • Two tasks that make up 25% of GCSE marks • An unaided observation and an aided observation chosen from the approved list • Unaided and aided observations can’t be from same row of approved list • If more than one task completed the best mark counts • Each task ...
... GCSE Astronomy Controlled Assessment • Two tasks that make up 25% of GCSE marks • An unaided observation and an aided observation chosen from the approved list • Unaided and aided observations can’t be from same row of approved list • If more than one task completed the best mark counts • Each task ...
RealOccult - Montgomery College
... • Moon traveling in it orbit around the earth occults stars. • When it occurs near the top or bottom of the moon this is called a Grazing Lunar Occultation. As the star gazes behind the lunar edge profile the star appears to go out and then back on when it appears from a deep lunar valley. • Grazing ...
... • Moon traveling in it orbit around the earth occults stars. • When it occurs near the top or bottom of the moon this is called a Grazing Lunar Occultation. As the star gazes behind the lunar edge profile the star appears to go out and then back on when it appears from a deep lunar valley. • Grazing ...
December, 2012 Vol.23 No.12 The Newsletter of the Cape Cod Astronomical Society
... Nicely high in the sky for much of the night, the king of planets will appear at its largest (49”) and brightest (mag -2.8) on that date. Don’t forget the Galilean moons; see our resource listings below for moon locations for any date and time. ...
... Nicely high in the sky for much of the night, the king of planets will appear at its largest (49”) and brightest (mag -2.8) on that date. Don’t forget the Galilean moons; see our resource listings below for moon locations for any date and time. ...
The Solar System - RHIG - Wayne State University
... principle? Can you give an example of a modern day theory where simplicity and elegance are the primary justifications? Q8. It is also a valid scientific principle to stick to tried-but-true models that explain all observations. Nobody wants to waste effort on wrong theories. Can you name a few exci ...
... principle? Can you give an example of a modern day theory where simplicity and elegance are the primary justifications? Q8. It is also a valid scientific principle to stick to tried-but-true models that explain all observations. Nobody wants to waste effort on wrong theories. Can you name a few exci ...
PDF, 95k
... 3 History of transit observations The transits of 6 June 1761 and 3 June 1769 were marked by major international observational campaigns involving many locations around the world. The first person to observe a transit of Venus was Jeremiah Horrocks in 1639. He envisaged using the transit to calculat ...
... 3 History of transit observations The transits of 6 June 1761 and 3 June 1769 were marked by major international observational campaigns involving many locations around the world. The first person to observe a transit of Venus was Jeremiah Horrocks in 1639. He envisaged using the transit to calculat ...
Word, 160 k
... Seen from the Earth on 8 June 2004, Venus will subtend an apparent diameter of about one arc minute. Thus our sister planet will be seen easily without an instrument and will be comparable in size to large sunspots. However, without an instrument it is hopeless to try to make valuable useful timings ...
... Seen from the Earth on 8 June 2004, Venus will subtend an apparent diameter of about one arc minute. Thus our sister planet will be seen easily without an instrument and will be comparable in size to large sunspots. However, without an instrument it is hopeless to try to make valuable useful timings ...
Part 2 - Hewlett
... Moon is closer to Earth than Sun. ______________________________________________________________________________ 13. Approximately how much time is there between consecutive high tides? ____________________ 12 hours 26 min 14. Why are there so many more impact craters on the Moon than on Earth? ____ ...
... Moon is closer to Earth than Sun. ______________________________________________________________________________ 13. Approximately how much time is there between consecutive high tides? ____________________ 12 hours 26 min 14. Why are there so many more impact craters on the Moon than on Earth? ____ ...
The Celestial Sphere
... Except the points directly above the north and south poles which do not appear to move. The sphere spins around them. They are called the North and South Celestial Poles. Half-way between the poles, above the Equator, lies the Celestial Equator it spins the most. ...
... Except the points directly above the north and south poles which do not appear to move. The sphere spins around them. They are called the North and South Celestial Poles. Half-way between the poles, above the Equator, lies the Celestial Equator it spins the most. ...
Astronomy Merit Badge Workshop
... and note them below. Alternatively, do an internet search for constellations visible from your area at this time of year, pick out 10, and note them below. *Do an Internet search for “Star Finder” of “Planisphere.” There are several good templates on the Internet; all you need to construct your own ...
... and note them below. Alternatively, do an internet search for constellations visible from your area at this time of year, pick out 10, and note them below. *Do an Internet search for “Star Finder” of “Planisphere.” There are several good templates on the Internet; all you need to construct your own ...
Mirrored Image Sep06.pub - High Desert Astronomical Society
... Asteroid 6 Hebe (8.5mag) moves southward through southwestern Capricornus this month. On the night of September 15, it passes between two seventh magnitude stars. ...
... Asteroid 6 Hebe (8.5mag) moves southward through southwestern Capricornus this month. On the night of September 15, it passes between two seventh magnitude stars. ...
Astronomy (ASTR)
... ASTR 390 Topics in Astronomy 3 Credit Hours A lecture in a topic of current interest in astronomy. Topics vary and are announced in the current Schedule of Classes. Three hours lecture. Prerequisite(s): ASTR 130 or PHYS 130 ASTR 390A Topics in Astronomy 3 Credit Hours Topic: Dark Mat ...
... ASTR 390 Topics in Astronomy 3 Credit Hours A lecture in a topic of current interest in astronomy. Topics vary and are announced in the current Schedule of Classes. Three hours lecture. Prerequisite(s): ASTR 130 or PHYS 130 ASTR 390A Topics in Astronomy 3 Credit Hours Topic: Dark Mat ...
Activities, In the Footsteps of Galileo
... of doubt to no one that they perform their revolutions about this planet while at the same time they all accomplish together orbits of twelve years’ length about the center of the world.” (Starry Messenger, Galileo Galilei, 1610) Objective: Discover that Jupiter exhibits a small, flattened disk as ...
... of doubt to no one that they perform their revolutions about this planet while at the same time they all accomplish together orbits of twelve years’ length about the center of the world.” (Starry Messenger, Galileo Galilei, 1610) Objective: Discover that Jupiter exhibits a small, flattened disk as ...
Astro 4 Practice Test 1
... a. It is a shape that people see and recognize in the sky, such as the `Big Dipper’. b. It is a cluster of stars that are all near each other in space. c. It is one of 88 regions in the sky with boundaries defined by the International Astronomical Union (IAU). d. It is one of about 10 regions in spa ...
... a. It is a shape that people see and recognize in the sky, such as the `Big Dipper’. b. It is a cluster of stars that are all near each other in space. c. It is one of 88 regions in the sky with boundaries defined by the International Astronomical Union (IAU). d. It is one of about 10 regions in spa ...
Archaeoastronomy
Archaeoastronomy (also spelled archeoastronomy) is the study of how people in the past ""have understood the phenomena in the sky, how they used these phenomena and what role the sky played in their cultures."" Clive Ruggles argues it is misleading to consider archaeoastronomy to be the study of ancient astronomy, as modern astronomy is a scientific discipline, while archaeoastronomy considers symbolically rich cultural interpretations of phenomena in the sky by other cultures. It is often twinned with ethnoastronomy, the anthropological study of skywatching in contemporary societies. Archaeoastronomy is also closely associated with historical astronomy, the use of historical records of heavenly events to answer astronomical problems and the history of astronomy, which uses written records to evaluate past astronomical practice.Archaeoastronomy uses a variety of methods to uncover evidence of past practices including archaeology, anthropology, astronomy, statistics and probability, and history. Because these methods are diverse and use data from such different sources, integrating them into a coherent argument has been a long-term difficulty for archaeoastronomers. Archaeoastronomy fills complementary niches in landscape archaeology and cognitive archaeology. Material evidence and its connection to the sky can reveal how a wider landscape can be integrated into beliefs about the cycles of nature, such as Mayan astronomy and its relationship with agriculture. Other examples which have brought together ideas of cognition and landscape include studies of the cosmic order embedded in the roads of settlements.Archaeoastronomy can be applied to all cultures and all time periods. The meanings of the sky vary from culture to culture; nevertheless there are scientific methods which can be applied across cultures when examining ancient beliefs. It is perhaps the need to balance the social and scientific aspects of archaeoastronomy which led Clive Ruggles to describe it as: ""...[A] field with academic work of high quality at one end but uncontrolled speculation bordering on lunacy at the other.""