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Chapter 1
Chapter 1

... Distances are so large in the universe that we can’t really use miles. Light years are just easier. It’s also interesting to think about the light we are seeing. For instance, when we look at things in the sky, we don’t actually see how they look right now; we see what they looked like. When we see ...
CHAPTER 20
CHAPTER 20

... In this chapter you will learn about all of the bodies of the solar system – the planets and their moons, asteroids, comets and meteoroids. You will also learn how space missions are making discoveries about our solar system that expand our knowledge of the solar neighborhood in which we live. ...
CHAPTER 20
CHAPTER 20

... In this chapter you will learn about all of the bodies of the solar system – the planets and their moons, asteroids, comets and meteoroids. You will also learn how space missions are making discoveries about our solar system that expand our knowledge of the solar neighborhood in which we live. ...
8th Grade Science Midterm Review Put all answers on a separate
8th Grade Science Midterm Review Put all answers on a separate

... section of the lab. It is also testable. For example is the question is, “Does texting negatively influence the time it takes to compete a Mario Kart course.” Then a good hypothesis would be “Sending a text message will increase the time it takes to complete a Mario Kart race.” Notice how the hypoth ...
PERMANENTLY SHADOWED AREAS AT THE LUNAR POLES
PERMANENTLY SHADOWED AREAS AT THE LUNAR POLES

... The polar areas are the unique terrain on the Moon. The orbital plane of the Moon is inclined to the plane of the ecliptic at an angle 5.13 . The regression of the line of nodes of the Moon’s orbit has amplitude of 9” in obliquity and varies over a period of 18.6 years. Taking account of these movem ...
8th Grade Science Midterm Review Put all answers on a separate
8th Grade Science Midterm Review Put all answers on a separate

... section of the lab. It is also testable. For example is the question is, “Does texting negatively influence the time it takes to compete a Mario Kart course.” Then a good hypothesis would be “Sending a text message will increase the time it takes to complete a Mario Kart race.” Notice how the hypoth ...
Falling Stars
Falling Stars

... who discovered it at the end of 1865.The scientists were not working together; one was in France and one was in America. They were each looking through telescopes. Both astronomers spotted the comet and reported their finding. The comet they found was not a big, bright comet. It is so small that it ...
Distribution of Elements in the Earth`s Crust
Distribution of Elements in the Earth`s Crust

... A supernova is the explosion of a star. A supernova occurs when a star exhausts all of its nuclear fuel and collapses. The collapse drives pressures and temperatures to levels so high that fusion reignites, forming elements heavier than iron, and the star explodes violently. Our solar system, planet ...
Why do we weigh more on Earth than on the moon?
Why do we weigh more on Earth than on the moon?

... then you’ve probably noticed the way they seemed to float from footstep to footstep. That’s because everything weighs less on the moon than it does on Earth. The reason for this has to do with gravity. Gravity is the force of attraction that exists between all objects in the universe, including Eart ...
Venus is a rocky planet very similar in size and surface gravity to
Venus is a rocky planet very similar in size and surface gravity to

... Venus spins even more slowly than Mercury, but it spins backwards as compared to its orbit around the Sun. The slow, backwards spin makes the Venusian day 177 Earth days long. Astronomers don't know for sure why Venus spins the way it does. The leading theory is that when Venus was a newly formed “p ...
Origin of Mountains and Primary Initiation of Submarine Canyons
Origin of Mountains and Primary Initiation of Submarine Canyons

... and high pressures from primordial Solar System gas under circumstances that isolated the condensate from further reaction with the gas at low temperatures [10, 14]. ...
October 2006 - Skyscrapers, Inc.
October 2006 - Skyscrapers, Inc.

... and metal. Most asteroids appear to be made of some combination of relatively heavy metals such as nickel and iron with some stone and carbonaceous material thrown in. [11, pages 113, 119, 131, 200, 204] Some theorists maintain that many if not most asteroids are what is left when all the ices in a ...
Celestial Events - Park Lane Learning Trust
Celestial Events - Park Lane Learning Trust

... Full Moon, Supermoon - The Moon will be located on the opposite side of the Earth as the Sun and its face will be will be fully illuminated. This is also the second of three supermoons for 2016. The Moon will be at its closest approach to the Earth and may look slightly larger and brighter than usua ...
Dawn Spacecraft Will Go Asteroid
Dawn Spacecraft Will Go Asteroid

... Dawn mission will help scientists understand the early stages of planet development. Scientists hope, for example, to gain insight into why the inner region of our solar system is composed of rocky planets and the outer, icy region is made up of gas giant planets. ...
Distance from the Sun
Distance from the Sun

... • Solar and lunar eclipses don't occur every month because the plane of the Moon's orbit around the Earth is not aligned with the plane of the Earth's orbit around the Sun. • The Moon's path is tilted when compared to the plane of Earth's orbit, so the Moon is not in a direct line with the Sun and E ...
Interplanetary Vagabonds
Interplanetary Vagabonds

... Asteroids also collide with each other breaking into fragments Fragments then travel together following the original orbits The groups of fragments are known as Hirayama Families If the relative velocity is high enough then the resulting fragments can be kicked out of asteroid area These fragments a ...
HOLIDAYS HOME WORK
HOLIDAYS HOME WORK

... Q5. A cubic millimeter of blood sample on microscopic examination is found to have 5 x 106 corpuscles. If an adult person contains 2.5 litres of blood, find the order of total number of red corpuscles in it. Q6. The diameter of a sphere is 2.34 cm. Calculate its surface area and the volume with due ...
Lec21_2D
Lec21_2D

...  With less CO2 in the atmosphere, the greenhouse effect was less effective  With more liquid water and a comfortable environment, photosynthetic life developed  Photosynthesis removed even more CO2 from the atmosphere, replacing it with O2. (When dinosaurs lived, there was 5 times more CO2 in the ...
Lunar Phases and Eclipses
Lunar Phases and Eclipses

... one nested inside the other. The outer or penumbral shadow is a zone where Earth blocks part but not all of the Sun’s rays from reaching the Moon. The inner or umbral shadow is a region where the Earth blocks all direct sunlight from reaching the Moon. ...
study-notes-for-2016-2017-1st-qtr-exam
study-notes-for-2016-2017-1st-qtr-exam

... and are considered “gas giants” because of their size and their primary make up of gases. Planets are big enough to other some smaller objects to revolve around them (moons) and to clear other larger objects from near their orbit. The Earth is the only planet/space object in our solar system known t ...
Earth`s Earliest Atmosphere
Earth`s Earliest Atmosphere

... This is sometimes taken to mean that Earth’s atmosphere degassed from the solid Earth into a primordial vacuum. However, most volatiles accreted by Earth as solids would have entered the atmosphere directly on impact (Ahrens et al. 1989). This would generally be the case for asteroids and meteors on ...
Earth`s Earliest Atmosphere
Earth`s Earliest Atmosphere

... This is sometimes taken to mean that Earth’s atmosphere degassed from the solid Earth into a primordial vacuum. However, most volatiles accreted by Earth as solids would have entered the atmosphere directly on impact (Ahrens et al. 1989). This would generally be the case for asteroids and meteors on ...
grade vii and viii - Sacred Heart CMI Public School
grade vii and viii - Sacred Heart CMI Public School

... sequence phase, from beginning to end, will last about 10 billion years for the Sun compared to around two billion years for all other phases of the Sun's pre-remnant life combined. Solar wind from the Sun created the heliosphere and swept away the remaining gas and dust from the proto planetary di ...
ASTR120 Homework 6 − Solutions
ASTR120 Homework 6 − Solutions

... a. Since Enceladus and Dione have a 1 : 2 ratio of orbital periods, the time between successive oppositions would be the orbital period of Dione -- 65.7 hours b. For this part, we want to use the small angle formula. According to the text, the linear diameter of Dione is 1.0 x 106 m. Enceladus is 2. ...
Gravity
Gravity

... On Earth, we have air. Air resistance will cause some objects to fall more slowly than others will. This works to our advantage when we want to fall more slowly, for example, when a skydiver jumps out of an airplane. He uses a parachute to create as much air resistance as possible to slow down his f ...
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Impact event



An impact event is a collision between celestial objects causing measurable effects. Impact events have physical consequences and have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal impact. When large objects impact terrestrial planets like the Earth, there can be significant physical and biospheric consequences, though atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid objects and present the strongest empirical evidence for their frequency and scale.Impact events appear to have played a significant role in the evolution of the Solar System since its formation. Major impact events have significantly shaped Earth's history, have been implicated in the formation of the Earth–Moon system, the evolutionary history of life, the origin of water on Earth and several mass extinctions. Notable impact events include the Chicxulub impact, 66 million years ago, believed to be the cause of the Cretaceous–Paleogene extinction event.Throughout recorded history, hundreds of Earth impacts (and exploding bolides) have been reported, with some occurrences causing deaths, injuries, property damage, or other significant localised consequences. One of the best-known recorded impacts in modern times was the Tunguska event, which occurred in Siberia, Russia, in 1908. The 2013 Chelyabinsk meteor event is the only known such event to result in a large number of injuries, and the Chelyabinsk meteor is the largest recorded object to have encountered the Earth since the Tunguska event.The most notable non-terrestrial event is the Comet Shoemaker–Levy 9 impact, which provided the first direct observation of an extraterrestrial collision of Solar System objects, when the comet broke apart and collided with Jupiter in July 1994. Most of the observed extrasolar impacts are the slow collision of galaxies; however, in 2014, one of the first massive terrestrial impacts observed was detected around the star NGC 2547 ID8 by NASA's Spitzer space telescope and confirmed by ground observations. Impact events have been a plot and background element in science fiction.
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