PDF file of Lecture 9a - Planet Jupiter
... Need to determine behavior of hydrogen and helium at high pressures and temperatures Correct for effects of pressure (conditions at Jupiter’s center: 25000 K and 100 Mbar) ...
... Need to determine behavior of hydrogen and helium at high pressures and temperatures Correct for effects of pressure (conditions at Jupiter’s center: 25000 K and 100 Mbar) ...
Prebiotic chemistry and the origin of life The early atmosphere of the
... oceans) starting from very simple molecules (H2, H2O, CH4, NH3) ...
... oceans) starting from very simple molecules (H2, H2O, CH4, NH3) ...
5.Rotational_P9sim_09
... 3. Kepler’s Laws of Planetary Motion (consequence of Newton’s Laws) 1. Planets move in elliptical orbits with the Sun at one focus. 2. A line from the sun to a planet sweeps out equal areas in a given period of time. 3. The square of the orbital period of a planet is proportional to the cube of its ...
... 3. Kepler’s Laws of Planetary Motion (consequence of Newton’s Laws) 1. Planets move in elliptical orbits with the Sun at one focus. 2. A line from the sun to a planet sweeps out equal areas in a given period of time. 3. The square of the orbital period of a planet is proportional to the cube of its ...
The Coriolis effect is a deflection of moving objects when
... reference, the Coriolis and centrifugal forces appear. Both forces are proportional to the mass of the object. The Coriolis force is proportional to the rotation rate, and the centrifugal force is proportional to its square. The Coriolis force acts in a direction perpendicular to the rotation axis a ...
... reference, the Coriolis and centrifugal forces appear. Both forces are proportional to the mass of the object. The Coriolis force is proportional to the rotation rate, and the centrifugal force is proportional to its square. The Coriolis force acts in a direction perpendicular to the rotation axis a ...
Theme 2.2 The Seasons The Sun`s Special Location In the previous
... In the previous unit we found it useful to begin with a situation in which we imagined the earth sitting alone in empty space, surrounded by a vast number of very distant stars. In fact, of course, the earth is very close to one star, the sun, which provides warmth, and gives us life. We will now co ...
... In the previous unit we found it useful to begin with a situation in which we imagined the earth sitting alone in empty space, surrounded by a vast number of very distant stars. In fact, of course, the earth is very close to one star, the sun, which provides warmth, and gives us life. We will now co ...
File
... satellite." • 3. Small solar system bodies: All other objects orbiting the sun • The Pluto issue will continue to play out for some time & is not yet settled ...
... satellite." • 3. Small solar system bodies: All other objects orbiting the sun • The Pluto issue will continue to play out for some time & is not yet settled ...
Beyond Planet Earth: Activities for Grades 6-8
... When our solar system began to take shape some 4.6 billion years ago, the Sun and planets as we know them today did not exist. Instead, a large disk of gas and dust known as the solar nebula swirled around a developing Sun. Within this disk, countless small objects collided and stuck together, gradu ...
... When our solar system began to take shape some 4.6 billion years ago, the Sun and planets as we know them today did not exist. Instead, a large disk of gas and dust known as the solar nebula swirled around a developing Sun. Within this disk, countless small objects collided and stuck together, gradu ...
Mercury - E
... other planets inside of it, and is thus the biggest planet in our Solar System. Jupiter has a streaky appearance because of the strong winds that are blowing the gases in an east to west direction. One of the interesting features on Jupiter is its “Giant Red Spot” – a hurricane or storm of swirling ...
... other planets inside of it, and is thus the biggest planet in our Solar System. Jupiter has a streaky appearance because of the strong winds that are blowing the gases in an east to west direction. One of the interesting features on Jupiter is its “Giant Red Spot” – a hurricane or storm of swirling ...
The Inner Planets
... • Venus’s atmosphere is mostly carbon dioxide- so you would not be able to breathe. Venus’s Rotation- a day is longer than a year on Venus!!! • Venus takes 7.5 Earth months to revolve around the sun(a year). • Venus takes 8 months to rotate once on its axis (a day). • Venus rotates from east to west ...
... • Venus’s atmosphere is mostly carbon dioxide- so you would not be able to breathe. Venus’s Rotation- a day is longer than a year on Venus!!! • Venus takes 7.5 Earth months to revolve around the sun(a year). • Venus takes 8 months to rotate once on its axis (a day). • Venus rotates from east to west ...
ppt
... • In addition there is a small particle • The barycenter is between mp and mq • The system is rotating at a uniform rate • Equations of motion include “frame” terms as a result of this rotation ...
... • In addition there is a small particle • The barycenter is between mp and mq • The system is rotating at a uniform rate • Equations of motion include “frame” terms as a result of this rotation ...
Advertising - Science Outreach
... http://www.spaceweathercenter.org/education/01/01.html This website has a range of resources on the Sun and space weather. There are many excellent pictures highlighting the various features of the Sun such as magnetic loops and coronal mass ejections (CMEs). The site also discusses space weather an ...
... http://www.spaceweathercenter.org/education/01/01.html This website has a range of resources on the Sun and space weather. There are many excellent pictures highlighting the various features of the Sun such as magnetic loops and coronal mass ejections (CMEs). The site also discusses space weather an ...
What`s Up In Space?
... 9. Read the following sentence. Most stars look tiny and can be seen only at night because they are so far away. Answer the following questions based on the information provided in the sentence you just read. One of the questions has already been answered for you. What is the main subject of the sen ...
... 9. Read the following sentence. Most stars look tiny and can be seen only at night because they are so far away. Answer the following questions based on the information provided in the sentence you just read. One of the questions has already been answered for you. What is the main subject of the sen ...
How to Make a Solar System Necklace
... equal to the mean distance between the Earth and the Sun (92,900,836.17 mi or 149,598,770 km). Most people might be familiar with the rough approximation of 93 million miles. This number is good for making rough conversions as long as you are not using the figure for something important, like a scho ...
... equal to the mean distance between the Earth and the Sun (92,900,836.17 mi or 149,598,770 km). Most people might be familiar with the rough approximation of 93 million miles. This number is good for making rough conversions as long as you are not using the figure for something important, like a scho ...
Solar system - Institute of Astronomy
... ecliptic (which is the plane of Earth’s orbit) • This rotation is just a small fraction of the angular momentum of the solar system (most of which is in the gas giant planets) ...
... ecliptic (which is the plane of Earth’s orbit) • This rotation is just a small fraction of the angular momentum of the solar system (most of which is in the gas giant planets) ...
Chapter 7 Circular Motion and Gravitation 7.1 Calculate force of
... 7.8 Conceptually relate mass and distance separation to the gravitational force, field strength, orbiting velocity and period of orbit for planetary bodies. 15. The only factor that affects the Earth’s gravitational force of attraction on objects at or near the Earth’s surface is the mass of the Ea ...
... 7.8 Conceptually relate mass and distance separation to the gravitational force, field strength, orbiting velocity and period of orbit for planetary bodies. 15. The only factor that affects the Earth’s gravitational force of attraction on objects at or near the Earth’s surface is the mass of the Ea ...
Kepler
... predictions: no better than Ptolemy’s • distance from Earth to celestial sphere is MUCH greater than Earth-Sun distance – explains why no parallax observed ...
... predictions: no better than Ptolemy’s • distance from Earth to celestial sphere is MUCH greater than Earth-Sun distance – explains why no parallax observed ...
Saturn - Otterbein University
... – Predicted from observed perturbations of Uranus's orbit: Adams (1845) and Leverrier (1846) – Observed by Galle (1846) ...
... – Predicted from observed perturbations of Uranus's orbit: Adams (1845) and Leverrier (1846) – Observed by Galle (1846) ...
Frequency Analysis
... The Lyapunov exponent can be computed numerically by following nearby trajectories with SwIFT, but problems may occur since d(t) must be infinitesimally small. (These problems can be avoided by using renormalization or variational equations.) Also, for a random choice of the initial orientation of t ...
... The Lyapunov exponent can be computed numerically by following nearby trajectories with SwIFT, but problems may occur since d(t) must be infinitesimally small. (These problems can be avoided by using renormalization or variational equations.) Also, for a random choice of the initial orientation of t ...
03/13/15 Astronomy
... Measuring Distances • Parallax – apparent change in position of an object when you look at it from a different position. ...
... Measuring Distances • Parallax – apparent change in position of an object when you look at it from a different position. ...
general information on uranus
... Venus is the __________________________________ in our solar system. It is the __________________________ in our Solar System. This planet is covered with fast-moving _______________________________ which trap heat from the Sun. Its _______________________________________________________. Ve ...
... Venus is the __________________________________ in our solar system. It is the __________________________ in our Solar System. This planet is covered with fast-moving _______________________________ which trap heat from the Sun. Its _______________________________________________________. Ve ...
Day 12 - Ch. 5 - Mercury and Venus
... Theories of the origin of the Terrestrials The “rocky” planets all formed in a warmer environment near the Sun in the early solar nebula. Current theories are based on computer models, which show that the inner planets formed from a band of planetesimals that may have been influenced by a Jupiter w ...
... Theories of the origin of the Terrestrials The “rocky” planets all formed in a warmer environment near the Sun in the early solar nebula. Current theories are based on computer models, which show that the inner planets formed from a band of planetesimals that may have been influenced by a Jupiter w ...
Neptune - Peterborough Astronomical Association
... retrograde motion, this peculiarity is one of the reasons astronomers think that it is a member of the Kuiper Belt which was gravitationally captured by Neptune. Like Earth’s Moon, Triton is tidally locked to Neptune. What that means is that the gravitational pull of Neptune has gradually slowed Tr ...
... retrograde motion, this peculiarity is one of the reasons astronomers think that it is a member of the Kuiper Belt which was gravitationally captured by Neptune. Like Earth’s Moon, Triton is tidally locked to Neptune. What that means is that the gravitational pull of Neptune has gradually slowed Tr ...
ISP 205: Visions of the Universe
... – The observable universe is 14 billion lightyears in radius and contains over 100 billion galaxies with a total number of stars comparable to the number of grains of sand on all of Earth’s beaches • How do our lifetimes compare to the age of the ...
... – The observable universe is 14 billion lightyears in radius and contains over 100 billion galaxies with a total number of stars comparable to the number of grains of sand on all of Earth’s beaches • How do our lifetimes compare to the age of the ...
27.1 Notes - MrPetersenScience
... • __________ a celestial body that orbits the sun, is round because of its own gravity, and has cleared the neighborhood around its orbital path • In the 1600s and 1700s, many scientists thought that the sun formed _______ and threw off the materials that later formed the _________. This was incorre ...
... • __________ a celestial body that orbits the sun, is round because of its own gravity, and has cleared the neighborhood around its orbital path • In the 1600s and 1700s, many scientists thought that the sun formed _______ and threw off the materials that later formed the _________. This was incorre ...
Ch. 27 The Planets in our Solar System
... • Meteorite – part of a large meteoroid that survives its trip through the atmosphere and strike’s Earth’s surface. (can consist of silicates, iron, nickel) – Impact Crater – bowl-shapped depression that remains after a meteorite has hit Earth, another planet, or a moon. • Rare on Earth – our atmosp ...
... • Meteorite – part of a large meteoroid that survives its trip through the atmosphere and strike’s Earth’s surface. (can consist of silicates, iron, nickel) – Impact Crater – bowl-shapped depression that remains after a meteorite has hit Earth, another planet, or a moon. • Rare on Earth – our atmosp ...
Earth's rotation
Earth's rotation is the rotation of the planet Earth around its own axis. The Earth rotates from the west towards east. As viewed from North Star or polestar Polaris, the Earth turns counter-clockwise.The North Pole, also known as the Geographic North Pole or Terrestrial North Pole, is the point in the Northern Hemisphere where the Earth's axis of rotation meets its surface. This point is distinct from the Earth's North Magnetic Pole. The South Pole is the other point where the Earth's axis of rotation intersects its surface, in Antarctica.The Earth rotates once in about 24 hours with respect to the sun and once every 23 hours 56 minutes and 4 seconds with respect to the stars (see below). Earth's rotation is slowing slightly with time; thus, a day was shorter in the past. This is due to the tidal effects the Moon has on Earth's rotation. Atomic clocks show that a modern-day is longer by about 1.7 milliseconds than a century ago, slowly increasing the rate at which UTC is adjusted by leap seconds.