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All about Venus! - Lunar and Planetary Institute
All about Venus! - Lunar and Planetary Institute

... All about Venus! Venus is the second planet from the Sun and is the sixth largest planet. It is about 95% the diameter of Earth. Venus has no moons. A Venusian day is 243 Earth days long - longer than its year of 225 days! Venus can be seen in the night sky with the naked eye. It is often called the ...
CH 27 PPT
CH 27 PPT

... • Orbits the Sun in 687 Earth days. • Rotates once in just over 24 Earth hours. • About one-half the diameter of Earth. • Gravity is only about 2/5 that of Earth. • Has a very weak or non-existent magnetic field. • Has a tilt similar to Earth (almost the same angle and in the same direction), giving ...
Solar System
Solar System

... -Since prehistoric times it has been known at a bright “wandering star”. ...
The Ocean-Atmosphere System
The Ocean-Atmosphere System

... Weather is the condition of the atmosphere at a particular time and place. It refers to such conditions of the local atmosphere as temperature, atmospheric pressure, humidity (the amount of water contained in the atmosphere), precipitation (rain, snow, sleet, & hail), and wind velocity. Because the ...
apparent magnitude
apparent magnitude

... The moons of the other planets range in size from very small to as large as terrestrial planets. All of the gas giants have multiple moons, and scientists are still discovering new moons. Some moons have very elongated, or elliptical, orbits, and some moons even orbit their planet ...
ten physics facts – setting the record straight
ten physics facts – setting the record straight

... warmer and the upper atmosphere cooler than it would be otherwise. Thus the familiar experience of cooler temperatures as you climb in altitude, a phenomenon called the lapse rate. Theory also has it, then, that an increase of gases like carbon dioxide will cause this thermal discontinuity to increa ...
Red Giants
Red Giants

... Eventually, the layer just outside the core called the ``shell layer'' gets hot and dense enough for fusion to start. The fusion in the layer just outside the core is called shell burning. This fusion is very rapid because the shell layer is still compressing and increasing in temperature. The lumin ...
The Greenhouse Effect
The Greenhouse Effect

... conduction and convection • Liquid water absorbs energy, changes into water vapor and the energy is then carried into the atmosphere ...
Climate models and assessment of climate change
Climate models and assessment of climate change

... Numerical weather prediction: –Initial state is critical –Don’t care about entire distribution, just most likely event –Need not conserve mass and energy ...
Where Did Everyone Go!
Where Did Everyone Go!

... In fact, there haven't been any around for about 66 million years. ...
ASTR-1020: Astronomy II Course Lecture Notes - Faculty
ASTR-1020: Astronomy II Course Lecture Notes - Faculty

... e) There is no magic going on here, just chemistry being powered by an energy source (i.e., the Sun). Mutations from cosmic rays and the UV radiation from the Sun cause further alterations to these long molecule chains =⇒ variation in lifeforms begin on Earth. Natural selection begins in earnest cau ...
NEXT MEETING THURSDAY, 18 th October 2012
NEXT MEETING THURSDAY, 18 th October 2012

... further. Launched on April 6, 1973, it reached Saturn early September, 1979 after using Jupiter for a gravity assist in December 1974. Voyagers 1 and 2 were the pinnacle of deep Solar System exploration. By fortunate coincidence, Jupiter, Saturn Uranus and Neptune were in the right configuration for ...
Atmosphere and Climate Change Section 2 Atmosphere Web quest
Atmosphere and Climate Change Section 2 Atmosphere Web quest

... • There will be more global warming is in our future according to the results of computer models summarized by the IPCC. For the next two decades warming of about 0.2° Celsius is projected. If we continue to emit as many, or more, greenhouse gases, this will cause more warming during the 21st Centur ...
Outer or Jovian Planets - Academic Computer Center
Outer or Jovian Planets - Academic Computer Center

... • Galileo Orbiter & Probe (1995-2003) • Voyager 1 & 2- Mission to Jupiter (1979), Saturn, Uranus, Neptune, and beyond • Ulysses - (1992- present) Mission to study the Sun via Jupiter • Pioneer 10 & 11(flyby 1973, 1974) ...
Teacher notes and student sheets
Teacher notes and student sheets

... Since the 1990s, very many ‘exoplanets’ have been found. It is estimated that much more than 10% of Sun-like stars have planets in orbit around them. Not all of these planets are suitable for life. Make an estimate of fL. Complex chemicals exist in much of the Universe. The development of simple liv ...
Chapter 3 The vertical structure of the atmosphere
Chapter 3 The vertical structure of the atmosphere

... (including us) from the damaging effects of this radiation. The stratosphere, as its name suggests, is highly stratified, poorly mixed (stratus meaning layered) with long residence times for particles ejected into it (for example by volcanos) from the troposphere below. It is close to radiative equil ...
ppt - Faculty Virginia
ppt - Faculty Virginia

... Jupiter and Saturn are. - The significant portion of their mass likely made up by water leads to Uranus and Neptune being called “ice giants” ...
Factors that Affect Air Pressure
Factors that Affect Air Pressure

... the surface, there are more air molecules, so pressure is greater. ...
Our Solar System
Our Solar System

... The sun is just a medium sized star (yellow dwarf). It is about 1.4 million kilometers in diameter It would take 10 Jupiter’s or 109 Earths to fit across the Sun! Makes life on our planet possible by giving us great amounts of light and heat. ...
Environmental Chemistry web
Environmental Chemistry web

... changes each day relatively small. For example, on the moon, the temperature changes from 123°C (253°F) during the day to -153°C (-243°F) at night. ...
Venus
Venus

... Venus is known as the morning star. It is also the brightest planet since it is close to the sun. Most of atmosphere is almost made up of only carbon dioxide. Earth and Venus are like basically the same size. It is 7,522 miles wide last the temperature can be more ...
Exam 3
Exam 3

... The rings of all the Jovian planets are found near to the planet, while moons are found farther out. This is because a) moons which are too near the planet will be torn apart by differential gravity forces b) moons too close to the planet will colide with one another and break each other apart c) mo ...
Airzone newsletter April 2010
Airzone newsletter April 2010

... Deborah says the 2008 results were different from other years because of the large-scale weather patterns that were present at the time. “Certain weather conditions aggravate the air quality situation in winter, causing smoke to be trapped at the surface. These conditions include very cold overnight ...
Lucas_CVAQ_20100130
Lucas_CVAQ_20100130

... • Warming of global surface temperatures is a result of increases in atmospheric greenhouse gas concentrations • Anthropogenic activities are the major source for increases in atmospheric greenhouse gas concentration • Although a global phenomenon, we will experience local impacts • The western US h ...
ATMOSPHERE AND HYDROSPHERE
ATMOSPHERE AND HYDROSPHERE

... E. Insolation reaching the earth's surface is absorbed and becomes heat. This heat energy is radiated back into the atmosphere as long-wavelength infrared radiation. F. This long-wavelength infrared radiation is readily absorbed by atmospheric CO2 and water vapor, thus preventing its rapid escape in ...
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Extraterrestrial atmosphere

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