AstroProjectDay3
... and the Moon on May 6, 2010. The spacecraft was 183 million kilometers (114 million miles) from Earth at the time, farther than our average distance from the Sun (150 million kilometers, or 93 million miles) because Mercury and Earth were at different places in their orbits around the Sun. ...
... and the Moon on May 6, 2010. The spacecraft was 183 million kilometers (114 million miles) from Earth at the time, farther than our average distance from the Sun (150 million kilometers, or 93 million miles) because Mercury and Earth were at different places in their orbits around the Sun. ...
The most accepted theory of the origin of the solar system is the
... Stage Three 6 – Temperature differences between the warm inner regions and the cool outer regions of the disk determined what kinds of material could condense to form planets – this is referred to as the temperature-condensation sequence. (Condensation is the formation of solid or liquid particles f ...
... Stage Three 6 – Temperature differences between the warm inner regions and the cool outer regions of the disk determined what kinds of material could condense to form planets – this is referred to as the temperature-condensation sequence. (Condensation is the formation of solid or liquid particles f ...
Star Systems FINAL EXAM STUDY GUIDE
... -You should be able to recognize photographs of the major planets and the moons listed above taken from telescopes, satellite or probe images, or images from the surface. -Even though you wont be asked to identify images of them, you should know the names of Uranus’ and Pluto’s major Moons, as well ...
... -You should be able to recognize photographs of the major planets and the moons listed above taken from telescopes, satellite or probe images, or images from the surface. -Even though you wont be asked to identify images of them, you should know the names of Uranus’ and Pluto’s major Moons, as well ...
This Month In Astronomy - Astronomy Club of Virginia Tech
... above. These objects fell into this category due to their further distance from the Sun (from around 47 AU to, for some, 100 AU), and their extreme inclination when compared to the plane of planets. Despite being further away from Neptune, the orbital status of these scattered disk objects resulted ...
... above. These objects fell into this category due to their further distance from the Sun (from around 47 AU to, for some, 100 AU), and their extreme inclination when compared to the plane of planets. Despite being further away from Neptune, the orbital status of these scattered disk objects resulted ...
title of lesson plan - Discovery Education
... Begin by leading the class in creating a web of planet facts to tap students' prior knowledge of astronomy topics. When the web is as big as it's going to get, share some basic planet facts with your students: Mercury is closest to the sun, Venus is the hottest planet, Earth is mostly water, Mars is ...
... Begin by leading the class in creating a web of planet facts to tap students' prior knowledge of astronomy topics. When the web is as big as it's going to get, share some basic planet facts with your students: Mercury is closest to the sun, Venus is the hottest planet, Earth is mostly water, Mars is ...
GEOL3025, Section 030 Lecture #11 31 August 2007
... Ability to hold onto an atmosphere depends on planet’s mass & temperature Escape velocity: minimum velocity to escape the gravity of a plant ...
... Ability to hold onto an atmosphere depends on planet’s mass & temperature Escape velocity: minimum velocity to escape the gravity of a plant ...
NAME
... The inner planets have more moons than the outer planets. The outer planets are smaller and very rocky. The outer planets are all larger and orbit the sun slower ...
... The inner planets have more moons than the outer planets. The outer planets are smaller and very rocky. The outer planets are all larger and orbit the sun slower ...
SolarSystemScaleProject_05
... on a bicycle moving at a velocity of 20 km/hr? How long would that same trip take if you walked at a steady pace of 5 km/hr? What general conclusion can you make based on these calculations? 8. Use the distance between each planet and the Sun to calculate the circumference (C) of each orbit. Compare ...
... on a bicycle moving at a velocity of 20 km/hr? How long would that same trip take if you walked at a steady pace of 5 km/hr? What general conclusion can you make based on these calculations? 8. Use the distance between each planet and the Sun to calculate the circumference (C) of each orbit. Compare ...
Solar System PPT
... galaxies that make up the universe • Introduction to the Solar System – VIDEO CLIP ...
... galaxies that make up the universe • Introduction to the Solar System – VIDEO CLIP ...
1 - Humble ISD
... 33. What do we theorize that comets brought to Earth?Water & Organic compounds 34. What is another name for the objects that exist beyond the orbit of Neptune?TransNeptunian Objects 35. How do dwarf planets differ from regular planets?They have failed to clear their orbits of other objects 36. What ...
... 33. What do we theorize that comets brought to Earth?Water & Organic compounds 34. What is another name for the objects that exist beyond the orbit of Neptune?TransNeptunian Objects 35. How do dwarf planets differ from regular planets?They have failed to clear their orbits of other objects 36. What ...
The Solar System and its Planets
... IAU regulaKons require a name from creaKon mythology for objects with orbital stability beyond Neptune's orbit. (from Wikipedia entry about the dwarf planet) ...
... IAU regulaKons require a name from creaKon mythology for objects with orbital stability beyond Neptune's orbit. (from Wikipedia entry about the dwarf planet) ...
Unit: Southern Europe
... GLE 0507.6.2: I can use charts to locate and identify star patterns. This means I can use a star chart to identify constellations in the night’s sky throughout the year. I can explain why it is important to know the time of night, the time of year, and the latitude to correctly identify the constell ...
... GLE 0507.6.2: I can use charts to locate and identify star patterns. This means I can use a star chart to identify constellations in the night’s sky throughout the year. I can explain why it is important to know the time of night, the time of year, and the latitude to correctly identify the constell ...
The Outer Worlds
... gravitational energy that heats the planet’s core – Observations show that Neptune emits more energy than it receives from the Sun – Uranus radiates as much energy into space as it receives from the Sun, indicating no internal source of thermal energy ...
... gravitational energy that heats the planet’s core – Observations show that Neptune emits more energy than it receives from the Sun – Uranus radiates as much energy into space as it receives from the Sun, indicating no internal source of thermal energy ...
The structure and formation of the Solar System
... • All the material in the early solar system is not used up when planets are formed. • Left over stuff is still flying around out there – these asteroids, meteoroids and comets still make impacts. • The asteroid belt is a large collection of asteroids. A theory, which is most favoured, is that the p ...
... • All the material in the early solar system is not used up when planets are formed. • Left over stuff is still flying around out there – these asteroids, meteoroids and comets still make impacts. • The asteroid belt is a large collection of asteroids. A theory, which is most favoured, is that the p ...
1. The Solar System
... the second-smallest planet in the Solar System. Some of the meteorites found on Earth are actually pieces of Mars. Jupiter is the fifth planet from the sun. It is 142,984 km in diameter. That makes Jupiter the largest planet in the Solar System. It is so large that all of the other planets in the so ...
... the second-smallest planet in the Solar System. Some of the meteorites found on Earth are actually pieces of Mars. Jupiter is the fifth planet from the sun. It is 142,984 km in diameter. That makes Jupiter the largest planet in the Solar System. It is so large that all of the other planets in the so ...
level 1
... Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto, Proxima Centuri, Barnard’s Star ...
... Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto, Proxima Centuri, Barnard’s Star ...
THE SOLAR SYSTEM
... Jupiter is the largest planet in the Solar System. It takes Jupiter only 10 hours to rotate completely on its axis. It takes Jupiter 4,331 Earth days to complete its orbit around the Sun. Its diameter is 88,846 miles , more than 11 times that of Earth, and about one-tenth that of the sun. It would t ...
... Jupiter is the largest planet in the Solar System. It takes Jupiter only 10 hours to rotate completely on its axis. It takes Jupiter 4,331 Earth days to complete its orbit around the Sun. Its diameter is 88,846 miles , more than 11 times that of Earth, and about one-tenth that of the sun. It would t ...
Observing Planetary Motion 15.3 Directions: Following the
... Record your observations of the marble. 3. Place the water balloon in the center of the sheet. Let go of the balloon so that the top of the mouthpiece of the balloon is facing the ceiling. Record what the balloon does to the sheet of latex. 4. Roll the marble onto the sheet towards the edge of the h ...
... Record your observations of the marble. 3. Place the water balloon in the center of the sheet. Let go of the balloon so that the top of the mouthpiece of the balloon is facing the ceiling. Record what the balloon does to the sheet of latex. 4. Roll the marble onto the sheet towards the edge of the h ...
Our Solar System
... orbits of Mars and Jupiter. It is believed that the asteroids in the asteroid belt never formed a planet because of the gravity of nearby Jupiter kept pulling them apart. Today, millions of asteroids probably inhabit the asteroid belt, with many more scattered throughout the solar system. ...
... orbits of Mars and Jupiter. It is believed that the asteroids in the asteroid belt never formed a planet because of the gravity of nearby Jupiter kept pulling them apart. Today, millions of asteroids probably inhabit the asteroid belt, with many more scattered throughout the solar system. ...
157a_midterm_2016
... A telescope is orbiting Mars at 300 km altitude. The telescope lens diameter is 40 cm, the focal length is 120 cm, and the focal plane is 4 cm wide. The pixels in the detector are 10 microns on a side. Calculate the swath width, size of the pixels on the ground, and the number of pixels across the s ...
... A telescope is orbiting Mars at 300 km altitude. The telescope lens diameter is 40 cm, the focal length is 120 cm, and the focal plane is 4 cm wide. The pixels in the detector are 10 microns on a side. Calculate the swath width, size of the pixels on the ground, and the number of pixels across the s ...
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.