Teacher`s Guide - Discovery Education
... Find out how the solar system formed and observe a model illustrating its vast distances. The Planets Discover the differences between the inner and outer planets. Listen to scientists debate Pluto’s status as a planet, and observe photographs of Jupiter from spacecraft. Comets and Asteroid Check ou ...
... Find out how the solar system formed and observe a model illustrating its vast distances. The Planets Discover the differences between the inner and outer planets. Listen to scientists debate Pluto’s status as a planet, and observe photographs of Jupiter from spacecraft. Comets and Asteroid Check ou ...
HW #10 Solutions
... orbital planes of the planets are very nearly coincident and that the Solar System must look very flat from an outside edge-on view. 15. Why are Venus, and Mercury never seen at midnight while the other planets can be visible then? Venus, and Mercury are never seen at midnight because they have maxi ...
... orbital planes of the planets are very nearly coincident and that the Solar System must look very flat from an outside edge-on view. 15. Why are Venus, and Mercury never seen at midnight while the other planets can be visible then? Venus, and Mercury are never seen at midnight because they have maxi ...
Space Science - Madison County Schools
... maria – dark, flat areas formed from lava 3-4 billion years ago crater – large, round pits caused by impacts of meteoroids highlands – oldest, most highly-cratered regions on the Moon Nitty Gritty Science © 2015 ...
... maria – dark, flat areas formed from lava 3-4 billion years ago crater – large, round pits caused by impacts of meteoroids highlands – oldest, most highly-cratered regions on the Moon Nitty Gritty Science © 2015 ...
Document
... • We’ll come back to this when we look at why we have seasons (outside of California). For now, let’s take a break from Celestial Spheres and consider the Phases of the Moon… ...
... • We’ll come back to this when we look at why we have seasons (outside of California). For now, let’s take a break from Celestial Spheres and consider the Phases of the Moon… ...
Constellations activities (PDF 185KB)
... throughout the year. The constellation of Orion can be seen during summer evenings and the constellation of Scorpius is in the sky during winter evenings. Orion is found low in the eastern sky from December, sits overhead throughout February, and sinks low in the western sky come April. Scorpius ...
... throughout the year. The constellation of Orion can be seen during summer evenings and the constellation of Scorpius is in the sky during winter evenings. Orion is found low in the eastern sky from December, sits overhead throughout February, and sinks low in the western sky come April. Scorpius ...
relative size and distance
... – The Sun, Moon, planets, and stars appear to rise in the east, cross the meridian due south, and set toward the west. – Celestial objects are said to transit when the cross the celestial meridian in the southern sky. • This is when they are highest in the sky. ...
... – The Sun, Moon, planets, and stars appear to rise in the east, cross the meridian due south, and set toward the west. – Celestial objects are said to transit when the cross the celestial meridian in the southern sky. • This is when they are highest in the sky. ...
S1-4-05 - Seasonal Constelallations - Lesson
... that when the object enters the scope of the light, it enables our eye to perceive it as something other than black. This can be addressed in the classroom by using a flashlight and explaining how the light would be perceived from different viewpoints. We can also get the students to imagine, or eve ...
... that when the object enters the scope of the light, it enables our eye to perceive it as something other than black. This can be addressed in the classroom by using a flashlight and explaining how the light would be perceived from different viewpoints. We can also get the students to imagine, or eve ...
Astronomy Puzzle-1
... Answers of puzzle are hidden in the box. The answers are either vertical, horizontal, diagonal or in reverse order. Sample answer is shown in the puzzle. Clues 1. The Astronomy research institute set up by the University Grant Commission. 2. The research institution set up by the Department of Spac ...
... Answers of puzzle are hidden in the box. The answers are either vertical, horizontal, diagonal or in reverse order. Sample answer is shown in the puzzle. Clues 1. The Astronomy research institute set up by the University Grant Commission. 2. The research institution set up by the Department of Spac ...
Welcome! Astronomy 100 / 190Y Exploring the Universe (Section A)
... Called the MKS system (meter, kilogram, second); all other quantities defined as function of these l Very useful: different units are related by factors of 10: l ...
... Called the MKS system (meter, kilogram, second); all other quantities defined as function of these l Very useful: different units are related by factors of 10: l ...
The Sun and the Stars
... Aristarchus measured an angle of 87 degrees, placing the Sun approx. 20 times further away than the Moon. [The correct scaling is ~390]. Error most likely associated with determining precisely when Moon is half-illuminated. ...
... Aristarchus measured an angle of 87 degrees, placing the Sun approx. 20 times further away than the Moon. [The correct scaling is ~390]. Error most likely associated with determining precisely when Moon is half-illuminated. ...
Lecture 3
... Aristarchus measured an angle of 87 degrees, placing the Sun approx. 20 times further away than the Moon. [The correct scaling is ~390]. Error most likely associated with determining precisely when Moon is half-illuminated. ...
... Aristarchus measured an angle of 87 degrees, placing the Sun approx. 20 times further away than the Moon. [The correct scaling is ~390]. Error most likely associated with determining precisely when Moon is half-illuminated. ...
Lookback Time in Our Everyday Lives
... Novas and supernovas are astronomical events that have been recorded down through history. The remnants of some of these are now seen as glowing nebulae. Below is a list of some of these events, when they were seen on Earth, and when they actually occurred (taking into account the light time to get ...
... Novas and supernovas are astronomical events that have been recorded down through history. The remnants of some of these are now seen as glowing nebulae. Below is a list of some of these events, when they were seen on Earth, and when they actually occurred (taking into account the light time to get ...
Earth Science 24.3 The Sun
... Sunspots appear dark because of their temperature, which is about 1500 K less than that of the surrounding solar surface. If these dark spots were observed away from the sun, they would appear many times brighter than the full moon. ...
... Sunspots appear dark because of their temperature, which is about 1500 K less than that of the surrounding solar surface. If these dark spots were observed away from the sun, they would appear many times brighter than the full moon. ...
The Sun Video Focus Questions
... 28. The tilt of the Earth on its axis causes part of the earth to get either more or less direct sunlight. During winter, the tilt of the earth causes the area to get less sunlight and during summer it causes the area to get more sunlight. 29. Without the sun providing the earth with warmth and ligh ...
... 28. The tilt of the Earth on its axis causes part of the earth to get either more or less direct sunlight. During winter, the tilt of the earth causes the area to get less sunlight and during summer it causes the area to get more sunlight. 29. Without the sun providing the earth with warmth and ligh ...
The Sun
... the core and cooler gases move outward. The part of the Sun usually seen from Earth is the photosphere. The two outermost layers of the Sun, the chromosphere and the corona, are such thin layers of gas that they can only be seen during a total solar eclipse. The Sun is almost a perfect sphere, which ...
... the core and cooler gases move outward. The part of the Sun usually seen from Earth is the photosphere. The two outermost layers of the Sun, the chromosphere and the corona, are such thin layers of gas that they can only be seen during a total solar eclipse. The Sun is almost a perfect sphere, which ...
Foundations of Harappan Astronomy:
... In the present study we evaluate the foundations of the nature of astronomical observations and noting that would have interested them and are likely to be found in their archaeological records. 2. Discussion of Harappan Astronomy Parpola (1994; 198:210) has extensively speculated on the possible as ...
... In the present study we evaluate the foundations of the nature of astronomical observations and noting that would have interested them and are likely to be found in their archaeological records. 2. Discussion of Harappan Astronomy Parpola (1994; 198:210) has extensively speculated on the possible as ...
Scale in the Solar System
... far away. In 2003, when Mars was as close to Earth as it had been in 60,000 years, the Mars was still 35 million miles away. That’s more distance than it would be to fly to the Moon and back 75 times. You could fly from Los Angeles to New York and back every day and it would still take you 20 years ...
... far away. In 2003, when Mars was as close to Earth as it had been in 60,000 years, the Mars was still 35 million miles away. That’s more distance than it would be to fly to the Moon and back 75 times. You could fly from Los Angeles to New York and back every day and it would still take you 20 years ...
Toys Watch the Sky
... The Sun appears to move from east to west due to the rotation of the Earth in the opposite direction (west to east). The time of day at which shadows are shortest is the time when the Sun is due north, so the shortest shadow points in a north-south direction. Some children may find it hard to believ ...
... The Sun appears to move from east to west due to the rotation of the Earth in the opposite direction (west to east). The time of day at which shadows are shortest is the time when the Sun is due north, so the shortest shadow points in a north-south direction. Some children may find it hard to believ ...
discover the wonders above
... You’ll be able to see many of the features that we mention in the calendar by looking up to the night sky. However, using binoculars or a telescope will often give you a better view and we’ve noted when they’re required. Visit bbc.co.uk/stargazing to find more guides and content to help you get star ...
... You’ll be able to see many of the features that we mention in the calendar by looking up to the night sky. However, using binoculars or a telescope will often give you a better view and we’ve noted when they’re required. Visit bbc.co.uk/stargazing to find more guides and content to help you get star ...
Precession of the Equinoxes and its Importance in Calendar Making
... ent path of the Sun in the celestial sphere remains the same, the moon and the planets show some deviations in their motions. The moon and the planets move to some extent towards north and south of the ecliptic. This deviation for the moon does not exceed much more than 5 degrees, while the planets ...
... ent path of the Sun in the celestial sphere remains the same, the moon and the planets show some deviations in their motions. The moon and the planets move to some extent towards north and south of the ecliptic. This deviation for the moon does not exceed much more than 5 degrees, while the planets ...
Sample pages 2 PDF
... measured in angular units. The declination increases from 0 to 90◦ in the northern direction and decreases from 0 to −90◦ in the southern direction. Historically, the right ascension is measured in time units, dividing the great circle, 360◦ , into 24 hours. The right ascension increases from 0 to 2 ...
... measured in angular units. The declination increases from 0 to 90◦ in the northern direction and decreases from 0 to −90◦ in the southern direction. Historically, the right ascension is measured in time units, dividing the great circle, 360◦ , into 24 hours. The right ascension increases from 0 to 2 ...
11 Celestial Objects and Events Every Stargazer Should See
... hydrogen and helium gas and peppered with traces of ammonia, methane, and frozen water. Making its way around the Sun once every 29.5 years, Saturn has a diameter nearly ten times that of Earth. But it’s also ...
... hydrogen and helium gas and peppered with traces of ammonia, methane, and frozen water. Making its way around the Sun once every 29.5 years, Saturn has a diameter nearly ten times that of Earth. But it’s also ...
CONSTELLATIONS
... remain in a given constellation for several months while Mars can be found in different constellations throughout the year. Jupiter and Saturn are at much greater distances from Earth than Mars. Jupiter and Saturn move much more slowly against the background stars than does Mars. Mars’ orbit is rela ...
... remain in a given constellation for several months while Mars can be found in different constellations throughout the year. Jupiter and Saturn are at much greater distances from Earth than Mars. Jupiter and Saturn move much more slowly against the background stars than does Mars. Mars’ orbit is rela ...
holiday lights - Denver Astronomical Society
... Way rises to replace the galactic-center view of late summer that was arrayed around Sagittarius. Now we are looking through the thin outer part of our galaxy’s disk into the great beyond. There we find constellations like Cassiopeia, Perseus, Auriga and Cancer the Crab. Gemini and Orion lie on eith ...
... Way rises to replace the galactic-center view of late summer that was arrayed around Sagittarius. Now we are looking through the thin outer part of our galaxy’s disk into the great beyond. There we find constellations like Cassiopeia, Perseus, Auriga and Cancer the Crab. Gemini and Orion lie on eith ...