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Bringing E.T. into Your Classroom The Search for
Bringing E.T. into Your Classroom The Search for

... 4. Small diameter planets or large diameter planets. 5. Small mass planets or large mass planets. 6. Planets close to star or planets far from star. ...
Shoot for the Stars - North Carolina 4-H
Shoot for the Stars - North Carolina 4-H

... have watched planets in the night sky. The planets can be seen at night not because they produce their own light like the sun or stars, but because they can reflect light. Some of the planets, such as Mercury, Venus, Mars, Jupiter, and Saturn, can even be seen without the aid of a telescope. Other p ...
NS2-M3C16_-_Asteroids,_Comets,_and_Meteorites_Exam
NS2-M3C16_-_Asteroids,_Comets,_and_Meteorites_Exam

... Mythological figures The person or persons who first discovered them. Mountain ranges on Earth Great astronomers from history ...
1000 Yard Solar System Model Worksheet
1000 Yard Solar System Model Worksheet

... (1,200,000). This is the size in *feet*. We want the size in inches. So multiply the answer by 12 to get inches. The Sun has been computed for you as a check of your math. (bonus: notice a pattern to the answers? how can you simplify this step?) 5) You will be assigned to a team. Each team should fi ...
How to Find a Habitable Planet
How to Find a Habitable Planet

... of stabilizing feedbacks between atmospheric CO2 and climate • Bad things happen, though, to planets around stars much different from the Sun --F and A stars: high stellar UV fluxes, short main sequence lifetimes --Late K and M stars: tidal locking, stellar flares, initial volatile inventories? ...
Using an Orrery – teachers` guide
Using an Orrery – teachers` guide

... 1. The planets in alphabetical order are:Earth Jupiter Mars Mercury Neptune Pluto Saturn Uranus Venus Write them out in order from the planet nearest the Sun to the planet furthest away from the Sun. Answer: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto. 2. How long is a year ...
Analysis
Analysis

... DISTANCES FROM THE SUN ...
Universal Gravitation
Universal Gravitation

... This relationship states that the force of attraction is directly proportional to each of the two masses and inversely proportional to the distance squared between the point masses. The gravitational constant G has a value of 6.673 x 10-11 N*m2/kg2. The inverse square relationship means that as the ...
What is the Nice model? - Lunar and Planetary Institute
What is the Nice model? - Lunar and Planetary Institute

... satellites during the Late Heavy Bombardment appears to be about an order of magnitude smaller than assumed by, e.g., Barr and Canup (2010). In fact, Nimmo and Korycansky (2012) suggested that icy satellites such as Mimas could remain icy if the impact rate was reduced by a factor of ten or so. The ...
PowerPoint - Division for Planetary Sciences
PowerPoint - Division for Planetary Sciences

... A Planet Orbiting Two Suns • About 1000 planets have been discovered outside our own solar system • But do planets form only around single stars? About half of all stars form in groups of two or more. • NASA’s Kepler spacecraft has detected a Saturn-sized planet orbiting two stars - the first discov ...
Solar System Text - Spring Creek Elementary
Solar System Text - Spring Creek Elementary

... A planet--a celestial body that revolves around a star—does not give off its own light, and is larger than asteroids or comets. The planets of our solar system, in order from the Sun, are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. At one time, Pluto was also considered a plan ...
Planetary Taxonomy
Planetary Taxonomy

Lecture 4, PPT version
Lecture 4, PPT version

... Do you notice anything different about Mars when it is undergoing retrograde motion? (Assume all the individual exposures were the same length of time.) Retrograde motion is on the TOP part of the “loop” in the sky. ...
Our Solar System LEVELED BOOK • S www.readinga-z.com
Our Solar System LEVELED BOOK • S www.readinga-z.com

Narrat - ESA/Hubble
Narrat - ESA/Hubble

... In a way our solar neighbourhood changed in 2006, when one of our planetary neighbours, Pluto, was downgraded from a planet to a dwarf planet. When it’s closest to Earth, Pluto is still a whopping 4.28 billion kilometres away! To give you an idea of how far that is, NASA’s New Horizon’s spacecraft i ...
Our Solar System - Mrs. Carter
Our Solar System - Mrs. Carter

... The Moon is about one-fourth the size of Earth. It reflects light from the Sun onto us. Many scientists believe the Moon was originally a part of Earth and was broken off in an enormous space collision. Tests have shown that there is water ice on the Moon’s surface. Earth’s ocean tides are caused by ...
Which exoEarths should we search for life
Which exoEarths should we search for life

... life beyond the Earth. Unless we are fortunate enough to detect a signal broadcast by another civilization, or detect life in situ elsewhere in the solar system, our main route to search for life will be the study of exo-Earths: Earth-type planets orbiting distant stars. Although no such planets hav ...
Astronomy
Astronomy

... • Rotates on its side; once every 17 hours • Revolves once every 84 years • At least 11 rings and 22 moons ...
A NEW FAMILY OF PLANETS? “OCEAN
A NEW FAMILY OF PLANETS? “OCEAN

... 5. the atmosphere has a given surface temperature governed by the distance to the star and the Greenhouse Effect. Its composition results from volatile outgasing, photochemistry and atmosphere escape. It is made of N2 , H2O, and CO2; 6. only planets that have migrated into the "Habitable Zone" are c ...
The outer solar system has four giant planets.
The outer solar system has four giant planets.

... Saturn was the first planet known to have rings. A planetary ring is a wide, flat zone of small particles that orbit a planet. All four gas giants have rings around their equators. Saturn’s rings are made of chunks of water ice the size of a building or smaller. Larger chunks, considered to be tiny ...
The Size and Distance Scale Of The Solar System
The Size and Distance Scale Of The Solar System

... inner part of the solar system travel, and may have originated in the early years of our solar system. • Surveys of the outer part of the solar system, beyond the orbit of Pluto, have recently found several additional objects comparable to Pluto in size. • Most recently, an object apparently larger ...
Chapter 9
Chapter 9

... • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have several surface features that have yet to be explained ...
Week 5 File
Week 5 File

... Both  these  ways  of  thinking  give  rise  to  the  expressions  above.  (See  the  worked  example   in  the  on-­‐line  hand-­‐wriNen  notes).   ...
click here for scale model worksheet
click here for scale model worksheet

... Scale Model of Solar System: If the Sun was the size of a basketball, then…. ...
C472 Continuous Assessment: Essay #2
C472 Continuous Assessment: Essay #2

... planets where life evolves, the fraction of evolved planets evolving intelligent life and several factors relating to communicative ability. The first of these factors is relatively easily found to be around 100 billion, however the values of later factors are not so clear cut. ...
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Planets beyond Neptune



Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.
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