![Planet Mercury.](http://s1.studyres.com/store/data/001289595_1-64c9e679565127381166e2ed4ac29125-300x300.png)
Planet Mercury.
... Mercury is known as a terrestrial planet consisting of about 70% metallic and 30% silicate material. The surface of the planet is covered in craters much like those seen on Earth’s moon. This is a sign that Mercury has been geologically dormant for billions of years. Since Mercury’s orbit is w ...
... Mercury is known as a terrestrial planet consisting of about 70% metallic and 30% silicate material. The surface of the planet is covered in craters much like those seen on Earth’s moon. This is a sign that Mercury has been geologically dormant for billions of years. Since Mercury’s orbit is w ...
Planet Porfolio - Complete Project
... 16. The magnetic field on Mercury is very weak compared to that of Earth – it is only ________________ the strength. 17. Though weak, the magnetic field interacts with that of solar wind to create intense ___________________ _________________________________________ . 18. Mercury has been hit by man ...
... 16. The magnetic field on Mercury is very weak compared to that of Earth – it is only ________________ the strength. 17. Though weak, the magnetic field interacts with that of solar wind to create intense ___________________ _________________________________________ . 18. Mercury has been hit by man ...
Unit 11: Astronomy
... 2. Solar size units In this section, we will use the diameter of the sun to represent a unit of 1. We will call this unit the sun size unit. diameter of the sun = 1,392,000 km = 1 sun size unit = 1 SSU We can compare the size of other objects to the sun using the sun size unit. 1. How many sun size ...
... 2. Solar size units In this section, we will use the diameter of the sun to represent a unit of 1. We will call this unit the sun size unit. diameter of the sun = 1,392,000 km = 1 sun size unit = 1 SSU We can compare the size of other objects to the sun using the sun size unit. 1. How many sun size ...
ARibbon at the Solar Systems Edge
... The combined scattering and neutralization processes now observed at the Moon have implications for interactions with objects across the solar system, such as asteroids, Kuiper Belt objects and other moons. The plasma-surface interactions occurring within protostellar nebula, the region of space tha ...
... The combined scattering and neutralization processes now observed at the Moon have implications for interactions with objects across the solar system, such as asteroids, Kuiper Belt objects and other moons. The plasma-surface interactions occurring within protostellar nebula, the region of space tha ...
The Planets
... Moon formed this way Mars— 1. why is it red? 2. structures: Mountians (Olympus Mons), Valles Marineris, Tharsis Bulge 3. structures: ice caps and composition 4. fluctuation of color with seasons 5. presence of water? Evidence? Jupiter— 1. main gases 2. why does it have a banded appearance? layers of ...
... Moon formed this way Mars— 1. why is it red? 2. structures: Mountians (Olympus Mons), Valles Marineris, Tharsis Bulge 3. structures: ice caps and composition 4. fluctuation of color with seasons 5. presence of water? Evidence? Jupiter— 1. main gases 2. why does it have a banded appearance? layers of ...
The Prospective Aspect of the Cosmogonic Models in Laozi and T
... Differs from Astronomical Theory (2/3) 3. In the course of this interstellar cloud’s workings, it may touch the nebular boundary of a neighboring star system, with interactive effects that produce a revolving pattern. – Each clump of interstellar cloud may gain initial angular momentum and projectin ...
... Differs from Astronomical Theory (2/3) 3. In the course of this interstellar cloud’s workings, it may touch the nebular boundary of a neighboring star system, with interactive effects that produce a revolving pattern. – Each clump of interstellar cloud may gain initial angular momentum and projectin ...
11/11/08 Chapter 9 The Outer Worlds… Jupiter Jupiter Jupiter`s
... respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in erup ...
... respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in erup ...
Comet ISON - Lone Star Science with Mr. Zuber
... Comet C/2012 S1 (ISON) • ISON started its journey towards the Sun (out of the Oort Cloud) a few million years ago • Discovered by Russian astronomers, part of the ISON Project (International Scientific Optical Network) in September 2012. • Comet ISON is a sungrazer, a comet that travels close to th ...
... Comet C/2012 S1 (ISON) • ISON started its journey towards the Sun (out of the Oort Cloud) a few million years ago • Discovered by Russian astronomers, part of the ISON Project (International Scientific Optical Network) in September 2012. • Comet ISON is a sungrazer, a comet that travels close to th ...
planetinvasionwebquest[1]. - teachingandlearningwithtech
... What is the size of the planet? What is the length of days and years? Find 3 interesting facts about Jupiter. Find at least 1 similarity and one 1 difference between Jupiter and Earth. http://starchild.gsfc.nasa.gov/docs/StarChild/solar_system_level1/j upiter.html http://www.enchantedlearning.com/su ...
... What is the size of the planet? What is the length of days and years? Find 3 interesting facts about Jupiter. Find at least 1 similarity and one 1 difference between Jupiter and Earth. http://starchild.gsfc.nasa.gov/docs/StarChild/solar_system_level1/j upiter.html http://www.enchantedlearning.com/su ...
Neptune
... Kuiper Belt Objects have colors (and spectra) consistent with them being icy. They are probably planetesimals that formed within the Kuiper belt. The Kuiper belt Objects are scattered too thinly for them to have accreted into a larger body. ...
... Kuiper Belt Objects have colors (and spectra) consistent with them being icy. They are probably planetesimals that formed within the Kuiper belt. The Kuiper belt Objects are scattered too thinly for them to have accreted into a larger body. ...
The Jovian Planets
... did not know how large Jupiter was when they first named it. Jupiter is 10 times the size of Earth and 300 times in mass ...
... did not know how large Jupiter was when they first named it. Jupiter is 10 times the size of Earth and 300 times in mass ...
Earth Science Lesson 9: Earth`s History Earth looks very different
... interior so hard that the pressure swells. As Earth’s internal pressure grew, its temperature also rose. Radioactive decay: Radioactive decay releases heat, and early in the planet’s history there were many radioactive elements with short half lives. These elements long ago decayed into stable mat ...
... interior so hard that the pressure swells. As Earth’s internal pressure grew, its temperature also rose. Radioactive decay: Radioactive decay releases heat, and early in the planet’s history there were many radioactive elements with short half lives. These elements long ago decayed into stable mat ...
The Jovian Planets
... did not know how large Jupiter was when they first named it. Jupiter is 10 times the size of Earth and 300 times in mass ...
... did not know how large Jupiter was when they first named it. Jupiter is 10 times the size of Earth and 300 times in mass ...
Vedic Cosmography and Astronomy 1
... Here we should discuss a potential misunderstanding. We have stated that Vaiñëavas have traditionally made use of the astronomical siddhäntas and that both Çréla Prabhupäda and Çréla Bhaktisiddhänta Sarasvaté Öhäkura have referred to them. At the same time, we have pointed out that the authors of th ...
... Here we should discuss a potential misunderstanding. We have stated that Vaiñëavas have traditionally made use of the astronomical siddhäntas and that both Çréla Prabhupäda and Çréla Bhaktisiddhänta Sarasvaté Öhäkura have referred to them. At the same time, we have pointed out that the authors of th ...
20gasgiantmoons2s
... Chemicals in Titan’s Atmosphere Titan’s atmosphere also contains hydrocarbons (composed of H and C) and polymers (long chains of H, N and C) ...
... Chemicals in Titan’s Atmosphere Titan’s atmosphere also contains hydrocarbons (composed of H and C) and polymers (long chains of H, N and C) ...
THE SUN AND THE MOON
... Galileo spacecraft in 1992. Many large impact craters are visible (light-colored areas with radiating lines). Image courtesy of NASA. ...
... Galileo spacecraft in 1992. Many large impact craters are visible (light-colored areas with radiating lines). Image courtesy of NASA. ...
Mercury Article - Learning Management Systems
... has almost no atmosphere. As a result, meteorites do not burn up as they do in other planets’ atmospheres. The many craters on Mercury’s surface were caused by all the space objects that have hit it through the years. How Many Moons Does Mercury Have? Mercury does not have any moons because it is so ...
... has almost no atmosphere. As a result, meteorites do not burn up as they do in other planets’ atmospheres. The many craters on Mercury’s surface were caused by all the space objects that have hit it through the years. How Many Moons Does Mercury Have? Mercury does not have any moons because it is so ...
Note Packet
... in water. Minerals that were once dissolved are called __________________________ and ___________________________ Crystalline sedimentary rocks are made of only one _____________________ and are called ___________________________________ Examples include: ______________________ and _________________ ...
... in water. Minerals that were once dissolved are called __________________________ and ___________________________ Crystalline sedimentary rocks are made of only one _____________________ and are called ___________________________________ Examples include: ______________________ and _________________ ...
Document
... Understand that the sun is many thousands of times closer to the earth than any other star. Light from the sun takes a few minutes to reach the earth, but light from the next nearest star takes a few years to arrive. The trip to that star would take the fastest rocket thousands of years.
... Understand that the sun is many thousands of times closer to the earth than any other star. Light from the sun takes a few minutes to reach the earth, but light from the next nearest star takes a few years to arrive. The trip to that star would take the fastest rocket thousands of years.
PLANETS
... • Solar System prototypes: Jupiter, Saturn, (Uranus, Neptune: icy giants)... • Substantial gaseous envelopes • Masses of the order of Jupiter mass (Jovian planets) • In the Solar System, NOT same composition as Sun • Presence of gas implies formation while gas was still prevalent Cores: Gas giants m ...
... • Solar System prototypes: Jupiter, Saturn, (Uranus, Neptune: icy giants)... • Substantial gaseous envelopes • Masses of the order of Jupiter mass (Jovian planets) • In the Solar System, NOT same composition as Sun • Presence of gas implies formation while gas was still prevalent Cores: Gas giants m ...
Ch 21 Fossils and the Rock Record
... Mass Number: Combined number of protons and neutrons in the nucleus of an atom. ...
... Mass Number: Combined number of protons and neutrons in the nucleus of an atom. ...
THE CONTRIBUTIONS OF COMETS TO
... (Whipple 1950), it has become clear that a traditional comet is actually an ice-rich small body called the nucleus that has wandered close enough to the Sun to produce a coma and tail by sublimation. Millions if not billions of these icy nuclei form a spherical shell around the plane of the solar sy ...
... (Whipple 1950), it has become clear that a traditional comet is actually an ice-rich small body called the nucleus that has wandered close enough to the Sun to produce a coma and tail by sublimation. Millions if not billions of these icy nuclei form a spherical shell around the plane of the solar sy ...
Chapter 9
... • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in eruption by the passing Voyager II • The material in the geyser is thought to be a mixture of nitrogen, ice, and carbon compounds heated beneath the surface by sunlight until it ...
... • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in eruption by the passing Voyager II • The material in the geyser is thought to be a mixture of nitrogen, ice, and carbon compounds heated beneath the surface by sunlight until it ...
a geocentric orrery
... of Orrery. Rowley dubbed the device "The Orrery." Orreries rapidly became popular as both a teaching aid and as an opulent piece of furniture. At left, an early orrery dating from about 1750; made by Benjamin Cole and now owned by St. Andrews University in Scotland. ...
... of Orrery. Rowley dubbed the device "The Orrery." Orreries rapidly became popular as both a teaching aid and as an opulent piece of furniture. At left, an early orrery dating from about 1750; made by Benjamin Cole and now owned by St. Andrews University in Scotland. ...
Late Heavy Bombardment
![](https://commons.wikimedia.org/wiki/Special:FilePath/Lunar_cataclysm.jpg?width=300)
The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.