The Sun`s Exterior
... The gas in the Sun’s corona is so hot it can escape the Sun’s gravity far from the photosphere. This stream of hot gas from the corona is known as the solar wind. It is often “gusty” as it is hit with shock waves from solar flares and coronal mass ejections. At 1 AU from the Sun, the solar wind is t ...
... The gas in the Sun’s corona is so hot it can escape the Sun’s gravity far from the photosphere. This stream of hot gas from the corona is known as the solar wind. It is often “gusty” as it is hit with shock waves from solar flares and coronal mass ejections. At 1 AU from the Sun, the solar wind is t ...
Section 1 Characteristics of the Atmosphere
... Strato (Low clouds), Alto (middle clouds), Cirro (high clouds) Be able to identify weather associated with the various cloud types and which types of clouds are associated with the different fronts. Figure 8 page 427 Section 2 Air Masses and Fronts Air masses are large bodies of air with sim ...
... Strato (Low clouds), Alto (middle clouds), Cirro (high clouds) Be able to identify weather associated with the various cloud types and which types of clouds are associated with the different fronts. Figure 8 page 427 Section 2 Air Masses and Fronts Air masses are large bodies of air with sim ...
Exoplanets
... Origin • Probably exist due to inward “migration” during planet formation Effects • Sweep terrestrial planet material into the star as they migrate • Gas Giants near or inside the habitable zone make stable orbits for terrestrial planets difficult or impossible ...
... Origin • Probably exist due to inward “migration” during planet formation Effects • Sweep terrestrial planet material into the star as they migrate • Gas Giants near or inside the habitable zone make stable orbits for terrestrial planets difficult or impossible ...
Scientific Method
... • The principles & empirical processes of discovery & demonstration considered characteristic of or necessary for scientific investigation, generally involving a) The observation of phenomena b) The formation of a hypothesis concerning the phenomena c) Experimentation to demonstrate the truth or fal ...
... • The principles & empirical processes of discovery & demonstration considered characteristic of or necessary for scientific investigation, generally involving a) The observation of phenomena b) The formation of a hypothesis concerning the phenomena c) Experimentation to demonstrate the truth or fal ...
PhysicsSG-Gravitation-91109R
... crushing the atoms out of existence. Under these extreme conditions, the protons and electrons can be squeezed together to form neutrons. If the collapse is halted when the neutrons all come into contact with each other, the result is an object called a neutron star, an entire star consisting of sol ...
... crushing the atoms out of existence. Under these extreme conditions, the protons and electrons can be squeezed together to form neutrons. If the collapse is halted when the neutrons all come into contact with each other, the result is an object called a neutron star, an entire star consisting of sol ...
A WALK THROUGH THE SOLAR SYSTEM
... Ancient astronomers observed points of light that appeared to move among the stars, and they called these objects planets, meaning wanderers. They were named after Roman legends. Jupiter was the king of the gods, Mars the god of war, Mercury was messenger of the gods, Venus was the god of beauty, an ...
... Ancient astronomers observed points of light that appeared to move among the stars, and they called these objects planets, meaning wanderers. They were named after Roman legends. Jupiter was the king of the gods, Mars the god of war, Mercury was messenger of the gods, Venus was the god of beauty, an ...
Planet formation - problems and future
... planets and yet be thin enough for the residual matter to be blown away by the Sun as its energy output increased. A consensus theory of planetary formation is now to hand based on the nebular hypothesis. It envisages the gradual accretion of planets, moons, and smaller objects, from cosmic dust gra ...
... planets and yet be thin enough for the residual matter to be blown away by the Sun as its energy output increased. A consensus theory of planetary formation is now to hand based on the nebular hypothesis. It envisages the gradual accretion of planets, moons, and smaller objects, from cosmic dust gra ...
PHASES OF THE MOON
... Day and night occur on Earth because of the rotation of the Earth on its axis. The Earth takes 24 hours to rotate. The Earth rotates counterclockwise from West to East. This causes the Sun to look like it rises in the East and sets in the West. Only ½ of the Earth is facing the Sun at a time. ...
... Day and night occur on Earth because of the rotation of the Earth on its axis. The Earth takes 24 hours to rotate. The Earth rotates counterclockwise from West to East. This causes the Sun to look like it rises in the East and sets in the West. Only ½ of the Earth is facing the Sun at a time. ...
Planetary Info Questions
... 2. Thick clouds surround Venus. What are they made of and what color? 3. Describe the “greenhouse effect” that exists on Venus. 4. How hot does it get on Venus? 5. Describe characteristics of Venus such as its atmospheric pressure, winds, and volcanism. ...
... 2. Thick clouds surround Venus. What are they made of and what color? 3. Describe the “greenhouse effect” that exists on Venus. 4. How hot does it get on Venus? 5. Describe characteristics of Venus such as its atmospheric pressure, winds, and volcanism. ...
What is a Planet
... Average distance from Sun- 3.8 billion miles Temperature- -382°F Diameter- 1,432 miles 3 Moon- Charon (Diameter of 730 miles), Nix and Hydra Atmosphere- 99.97% Nitrogen Rotation= 6.38 days Revolution= 248.6 years Gravity- 1/8 that of Earth Orbit- Pluto has a more elliptical and titled orbit, one of ...
... Average distance from Sun- 3.8 billion miles Temperature- -382°F Diameter- 1,432 miles 3 Moon- Charon (Diameter of 730 miles), Nix and Hydra Atmosphere- 99.97% Nitrogen Rotation= 6.38 days Revolution= 248.6 years Gravity- 1/8 that of Earth Orbit- Pluto has a more elliptical and titled orbit, one of ...
Categorizing Solar System Objects
... Triton, satellite of Neptune – Triton is covered in ice and may have a weak atmosphere. Venus, planet – Vesta, asteroid – Vesta has an interesting surface with clear light and dark regions, unlike most other asteroids, meaning that it is made up of many different elements. Wild 2, comet – ...
... Triton, satellite of Neptune – Triton is covered in ice and may have a weak atmosphere. Venus, planet – Vesta, asteroid – Vesta has an interesting surface with clear light and dark regions, unlike most other asteroids, meaning that it is made up of many different elements. Wild 2, comet – ...
Ch 13 Smeopardy
... gases. O C) The outer planets are located in the asteroid belt. O D) Jupiter is the only outer planet that is small and rocky. ...
... gases. O C) The outer planets are located in the asteroid belt. O D) Jupiter is the only outer planet that is small and rocky. ...
Third Grade Science
... properties. P.2.3 Summarize changes that occur to the observable properties of materials when different degrees of heat are applied to them, such as melting ice or ice cream, boiling water or an egg, or freezing water. ...
... properties. P.2.3 Summarize changes that occur to the observable properties of materials when different degrees of heat are applied to them, such as melting ice or ice cream, boiling water or an egg, or freezing water. ...
Adventurer Pathfinder
... Galileo was the first person to use a telescope to explore the heavens. With the telescope, Galileo discovered that Jupiter had four moons. He also spent time observing our moon, star patterns, and sunspots. Galileo eventually went blind from looking at the sun through his telescope! Before 1700, pe ...
... Galileo was the first person to use a telescope to explore the heavens. With the telescope, Galileo discovered that Jupiter had four moons. He also spent time observing our moon, star patterns, and sunspots. Galileo eventually went blind from looking at the sun through his telescope! Before 1700, pe ...
Carter K 1 - Mrs. Anthony`s English 2
... was taken into consideration for all three planets, it was concluded that all three of these planets are very earthlike and have a high possibility of life. Not on the whole planet though, all three planets are tidally locked, meaning one side is always facing the sun and the other is not. With this ...
... was taken into consideration for all three planets, it was concluded that all three of these planets are very earthlike and have a high possibility of life. Not on the whole planet though, all three planets are tidally locked, meaning one side is always facing the sun and the other is not. With this ...
Earth Science Chapter 24 File
... waves on an antenna, which absorbs and transmits theses waves to an amplifier, just like a radio antenna Can be used at any time of the day and in any weather, but they are limited by man-made radio interference ...
... waves on an antenna, which absorbs and transmits theses waves to an amplifier, just like a radio antenna Can be used at any time of the day and in any weather, but they are limited by man-made radio interference ...
ASTRONOMY 4
... T F 36) According to the nebular hypothesis, the Sun should have most of the angular momentum of the Solar System, but it doesn't. T F 37) According to the nebular hypothesis, the planets should have most of the angular momentum of the Solar System, but they don't. T F 38) The Moon should be rotatin ...
... T F 36) According to the nebular hypothesis, the Sun should have most of the angular momentum of the Solar System, but it doesn't. T F 37) According to the nebular hypothesis, the planets should have most of the angular momentum of the Solar System, but they don't. T F 38) The Moon should be rotatin ...
4QA Jeopardy
... One piece of evidence used to back up the Big Bang was the Doppler Effect. What does the Doppler Affect show us? a.) Stars and Galaxies are moving away ...
... One piece of evidence used to back up the Big Bang was the Doppler Effect. What does the Doppler Affect show us? a.) Stars and Galaxies are moving away ...
Introduction to Basic Stargazing Part II - Naples Free-Net
... It is a peculiarity of comets that no matter where the comet is headed, the tail always points away from the Sun. Comets can also have two tails, one is of mostly dust, the other gas. Meteors: Remember all that dust and dirt the comets give off? It does not disappear, but continues to orbit the Sun ...
... It is a peculiarity of comets that no matter where the comet is headed, the tail always points away from the Sun. Comets can also have two tails, one is of mostly dust, the other gas. Meteors: Remember all that dust and dirt the comets give off? It does not disappear, but continues to orbit the Sun ...
Do the planets orbit the Sun at constant speeds?
... seen from Earth. In the Ptolemaic (geocentric) model, Venus would be seen in only new or crescent phases. However, as Galileo observed, Venus is seen in all phases, which agrees with the Copernican model as shown. ...
... seen from Earth. In the Ptolemaic (geocentric) model, Venus would be seen in only new or crescent phases. However, as Galileo observed, Venus is seen in all phases, which agrees with the Copernican model as shown. ...
Formation and evolution of the Solar System
The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.