FOSS Earth and Sun Module Glossary NGSS Edition © 2016 absorb
... planet a large, round object orbiting a star (SRB, IG) precipitation rain, snow, sleet, or hail that falls to the ground (SRB, IG) pressure the force or push caused by moving molecules (IG) radiant energy energy that travels through air and space (SRB, IG) radiation energy that travels through air ...
... planet a large, round object orbiting a star (SRB, IG) precipitation rain, snow, sleet, or hail that falls to the ground (SRB, IG) pressure the force or push caused by moving molecules (IG) radiant energy energy that travels through air and space (SRB, IG) radiation energy that travels through air ...
Galaxies - WordPress.com
... ones with large, bright nuclei of stars and tightly wound spiral arms, to ones with very small, dim nuclei and open sprawling arms. The Andromeda Galaxy is also a spiral galaxy. ...
... ones with large, bright nuclei of stars and tightly wound spiral arms, to ones with very small, dim nuclei and open sprawling arms. The Andromeda Galaxy is also a spiral galaxy. ...
Newton`s Law of Universal Gravitation
... 1. Suppose that two objects attract each other with a gravitational force of 16 units. If the distance between the two objects is doubled, what is the new force of attraction between the two objects? 2. Suppose that two objects attract each other with a gravitational force of 16 units. If the distan ...
... 1. Suppose that two objects attract each other with a gravitational force of 16 units. If the distance between the two objects is doubled, what is the new force of attraction between the two objects? 2. Suppose that two objects attract each other with a gravitational force of 16 units. If the distan ...
Stellar Evolution: Evolution: Birth, Life, and Death of Stars
... discovered and studied through gravitational effect they have on the star, or through the light dimming of its star if transit occur. Very few have been directly captured (left). Unlike the planets in our Solar System, many exoplanets are huge and very close to its star. This allows the astronomers ...
... discovered and studied through gravitational effect they have on the star, or through the light dimming of its star if transit occur. Very few have been directly captured (left). Unlike the planets in our Solar System, many exoplanets are huge and very close to its star. This allows the astronomers ...
TheExpansionoftheUniverse
... tired-light theory- this theory suggests that lost energy disappears from the universe completely-even tho it goes against the First Law of Thermodynamics; Paul LaViolette was one of the first people to disprove the expanding universe theory some of his work suggested cosmological red shift- which w ...
... tired-light theory- this theory suggests that lost energy disappears from the universe completely-even tho it goes against the First Law of Thermodynamics; Paul LaViolette was one of the first people to disprove the expanding universe theory some of his work suggested cosmological red shift- which w ...
The Dimensions Program - Asnuntuck Community College
... of, and approximately how much longer they will exist. When they do die out, astronomers can also tell how they die and what they will look like afterwards. Astronomy answers the question of what happens in the universe. An Optical Interferometer helps to figure out what is happing in the universe b ...
... of, and approximately how much longer they will exist. When they do die out, astronomers can also tell how they die and what they will look like afterwards. Astronomy answers the question of what happens in the universe. An Optical Interferometer helps to figure out what is happing in the universe b ...
Science-Map-Grade-4
... Predict the amount of mass in different items Calculate the volume of water and other objects Convert units of measurement in standard system Measure volume and mass Explain how matter changes from one state to another Illustrate what matter particles look like in the different phases of gas, liquid ...
... Predict the amount of mass in different items Calculate the volume of water and other objects Convert units of measurement in standard system Measure volume and mass Explain how matter changes from one state to another Illustrate what matter particles look like in the different phases of gas, liquid ...
Chapter 1 PowerPoint
... • How big is the universe? – The distances between planets are huge compared to their sizes—on a scale of 1-to-10-billion, Earth is the size of a ball point and the Sun is 15 meters away. – On the same scale, the stars are thousands of kilometers away. – It would take more than 3000 years to count t ...
... • How big is the universe? – The distances between planets are huge compared to their sizes—on a scale of 1-to-10-billion, Earth is the size of a ball point and the Sun is 15 meters away. – On the same scale, the stars are thousands of kilometers away. – It would take more than 3000 years to count t ...
SeagerGUASAI - Sara Seager
... exoplanets discussed the possibility of giving popular names to exoplanets in addition to their existing catalogue designation (for instance HD 85512 b). Although no consensus was reached, the majority was not in favour of this possibility at the time. However, considering the ever increasing intere ...
... exoplanets discussed the possibility of giving popular names to exoplanets in addition to their existing catalogue designation (for instance HD 85512 b). Although no consensus was reached, the majority was not in favour of this possibility at the time. However, considering the ever increasing intere ...
Ben R. Oppenheimer1,2 and Sasha Hinkley1,2
... (commonly defined as objects below roughly 13 MJ where MJ is the mass of Jupiter; see Side Bar), one need only take a very superficial look at the objects in our solar system to see a vast diversity. Indeed, the giant planets of our solar system are all roughly of the same radius, of nearly the sam ...
... (commonly defined as objects below roughly 13 MJ where MJ is the mass of Jupiter; see Side Bar), one need only take a very superficial look at the objects in our solar system to see a vast diversity. Indeed, the giant planets of our solar system are all roughly of the same radius, of nearly the sam ...
How Marius Was Right and Galileo Was Wrong Even Though
... these ideas will require further discussion and explanation. Lastly, he concedes to Galileo that the stars shine by their own light -- they are distinct in appearance from the planets (being notably more intense in brilliance).13 ...
... these ideas will require further discussion and explanation. Lastly, he concedes to Galileo that the stars shine by their own light -- they are distinct in appearance from the planets (being notably more intense in brilliance).13 ...
What is the “Meridian”?
... Right Ascension (Celestial Longitude, measured (angular distance from the “Vernal Equinox”) ...
... Right Ascension (Celestial Longitude, measured (angular distance from the “Vernal Equinox”) ...
Extrasolar Cosmochemistry
... We now consider the amount of mass required in our standard model; we argue that minor planets such as asteroids are the dominant source for the pollution of white dwarf atmospheres, although there might be instances in which tidal disruption and accretion of an entire planet the size of Mars has oc ...
... We now consider the amount of mass required in our standard model; we argue that minor planets such as asteroids are the dominant source for the pollution of white dwarf atmospheres, although there might be instances in which tidal disruption and accretion of an entire planet the size of Mars has oc ...
Read an Excerpt!
... 559 years to orbit the Sun. This period is more than twice as long as Pluto takes to orbit the Sun. On average, Eris is 6.3 billion (6,300,000,000) miles from the Sun—billions of miles beyond Pluto’s orbit. That’s 68 times farther than the Earth is. But the orbit of Eris around the Sun is weird. It’ ...
... 559 years to orbit the Sun. This period is more than twice as long as Pluto takes to orbit the Sun. On average, Eris is 6.3 billion (6,300,000,000) miles from the Sun—billions of miles beyond Pluto’s orbit. That’s 68 times farther than the Earth is. But the orbit of Eris around the Sun is weird. It’ ...
13 Unit 8 5th Grade Science
... characteristics of Earth that are necessary for life to exist, have students respond to a SPAWN prompt (view literacy strategy descriptions). SPAWN represents five categories of prompts: S (Special Powers), P (Problem Solving), A (Alternative Viewpoints), W (What If?) and N (Next). These prompts can ...
... characteristics of Earth that are necessary for life to exist, have students respond to a SPAWN prompt (view literacy strategy descriptions). SPAWN represents five categories of prompts: S (Special Powers), P (Problem Solving), A (Alternative Viewpoints), W (What If?) and N (Next). These prompts can ...
click here
... explaining why stars resided in different places, but at least the pattern that all agreed on made it clear that the quest would be ...
... explaining why stars resided in different places, but at least the pattern that all agreed on made it clear that the quest would be ...
- National Optical Astronomy Observatory
... method of image capture (CCD vs. photoelectric photometer). The distance to the cluster observed in del Rio’s paper also varies from the findings in this study (1230 pc versus 1400 pc) (1987), although not by a great deal. SUMMARY Using modern methods of photometry to analyze images taken of NGC 149 ...
... method of image capture (CCD vs. photoelectric photometer). The distance to the cluster observed in del Rio’s paper also varies from the findings in this study (1230 pc versus 1400 pc) (1987), although not by a great deal. SUMMARY Using modern methods of photometry to analyze images taken of NGC 149 ...
Chapter1 - A Modern View of the Univserse -pptx
... • How did we come to be? – The matter in our bodies came from the Big Bang, which produced hydrogen and helium. – All other elements were constructed from H and He in stars and then recycled into new star systems, including our solar system. • How do our lifetimes compare to the age of the universe? ...
... • How did we come to be? – The matter in our bodies came from the Big Bang, which produced hydrogen and helium. – All other elements were constructed from H and He in stars and then recycled into new star systems, including our solar system. • How do our lifetimes compare to the age of the universe? ...
Basics – II. Time, Magnitudes and Spectral types
... (along the celestial equator) we see a varying rate due to the projection of the ecliptic on to the celestial equator. This introduces a variation from uniform motion which is a wave of period half a year. The combination of these two effects leads to the Equation of Time (see figures). In effect, w ...
... (along the celestial equator) we see a varying rate due to the projection of the ecliptic on to the celestial equator. This introduces a variation from uniform motion which is a wave of period half a year. The combination of these two effects leads to the Equation of Time (see figures). In effect, w ...
ASTRONOMY REVIEW Qs - Westhampton Beach School District
... 29. Base your answer to the following question on the passage below. A Newly Discovered Planet Scientists studying a Sun-like star named Ogle-Tr-3 discovered a planet that is, on the average, 3.5 million kilometers away from the star’s surface. The planet was discovered as a result of observing a cy ...
... 29. Base your answer to the following question on the passage below. A Newly Discovered Planet Scientists studying a Sun-like star named Ogle-Tr-3 discovered a planet that is, on the average, 3.5 million kilometers away from the star’s surface. The planet was discovered as a result of observing a cy ...
Chemical Universe. - University of Texas Astronomy
... f the first three elements were made in the first three minutes, the rest didn’t come along until about a billion years later, with the formation of the first stars and galaxies. That’s because the other elements were forged in the universe’s chemical factories: the stars. Except for those created i ...
... f the first three elements were made in the first three minutes, the rest didn’t come along until about a billion years later, with the formation of the first stars and galaxies. That’s because the other elements were forged in the universe’s chemical factories: the stars. Except for those created i ...
Astro-2: History of the Universe
... Universe The Hubble constant gives us the current expansion rate of the universe, which we can use to estimate the age of the Universe. 1/H0 is approximately equal to 14 Gyr We should test whether this is consistent with the age of “stuff” in the universe. If we found something significantly older t ...
... Universe The Hubble constant gives us the current expansion rate of the universe, which we can use to estimate the age of the Universe. 1/H0 is approximately equal to 14 Gyr We should test whether this is consistent with the age of “stuff” in the universe. If we found something significantly older t ...
TAKS objective 5 Earth and Space Systems
... The Sun is a Star Our sun is a medium-size yellow star. It is 4.6 billion years old. In the sun, hydrogen undergoes nuclear fusion, a process that releases vast amounts of energy. During fusion hydrogen atoms join to form helium atoms. Hydrogen fusion is the source of light, heat, and other radiati ...
... The Sun is a Star Our sun is a medium-size yellow star. It is 4.6 billion years old. In the sun, hydrogen undergoes nuclear fusion, a process that releases vast amounts of energy. During fusion hydrogen atoms join to form helium atoms. Hydrogen fusion is the source of light, heat, and other radiati ...
PDF format
... • How big is the universe? – The distances between planets are huge compared to their sizes—on a scale of 1-to-10-billion, Earth is the size of a ball point and the Sun is 15 meters away. – On the same scale, the stars are thousands of kilometers away. – It would take more than 3000 years to cou ...
... • How big is the universe? – The distances between planets are huge compared to their sizes—on a scale of 1-to-10-billion, Earth is the size of a ball point and the Sun is 15 meters away. – On the same scale, the stars are thousands of kilometers away. – It would take more than 3000 years to cou ...
P7 Further Physics : Observing the Universe
... materials introduces atomic and nuclear structure, neutrons, and protons – but not the evidence for them. ...
... materials introduces atomic and nuclear structure, neutrons, and protons – but not the evidence for them. ...
Extraterrestrial life
Extraterrestrial life is life that does not originate from Earth. It is also called alien life, or, if it is a sentient and/or relatively complex individual, an ""extraterrestrial"" or ""alien"" (or, to avoid confusion with the legal sense of ""alien"", a ""space alien""). These as-yet-hypothetical life forms range from simple bacteria-like organisms to beings with civilizations far more advanced than humanity. Although many scientists expect extraterrestrial life to exist, so far no unambiguous evidence for its existence exists.The science of extraterrestrial life is known as exobiology. The science of astrobiology also considers life on Earth as well, and in the broader astronomical context. Meteorites that have fallen to Earth have sometimes been examined for signs of microscopic extraterrestrial life. Since the mid-20th century, there has been an ongoing search for signs of extraterrestrial intelligence, from radios used to detect possible extraterrestrial signals, to telescopes used to search for potentially habitable extrasolar planets. It has also played a major role in works of science fiction. Over the years, science fiction works, especially Hollywood's involvement, has increased the public's interest in the possibility of extraterrestrial life. Some encourage aggressive methods to try to get in contact with life in outer space, whereas others argue that it might be dangerous to actively call attention to Earth.