Kuiper Belt Jupiter Mercury Venus Urahus Saturn Mars Farth · Ceres Neptune Jupiter Pluto inner solar system outer solar system not to scale Is this model to scale regarding the sizes of the planets and distances between them? Why or why not? O Yes. That is why the outer planets are shown in a separate box. O No. The distances in the solar system are too great to produce a model accurate to distance that still has inner planets visible. No. The outer planet distances are drawn to scale, but the inner planets need to be drawn farther from the sun to be visible 1 4
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- Our Solar System consist of two distinctly different types of planets. A. Describe how these planets differ in their general characteristics. B. Explain the cause of these differences1- MODIS is an Earth Observation sensor onboard TERRA spacecraft flying in a near-polar circular orbit with an orbital period of 98.8 minutes. The width of the swath imaged by MODIS is 2330 km. A- How many orbits does TERRA trace in one day? B- Assuming that the Earth rotates around its polar axis at a rate of 0.2618 rd/hr and that the equatorial radius is 6378 km, do two consecutive swaths of MODIS overlap at the equator? (hint: the length of an arc = angle in rd * radius) C- The radius of the latitude circle at 35 deg is 5224.5 km. Do two consecutive swaths of MODIS overlap at latitude 35 deg? 2- An aerostationary orbit for Mars is equivalent to a geostationary orbit for Earth. It is designed to enable a satellite in that orbit to image always the same surface of Mars. Calculate the altitude of an aerostationary orbit assuming that Mars is spherical, that its sidereal rotational period is 1.02595676 Earth days, its equatorial radius is 3389.50 km and its mass is…Nearly all planets that astronomers have found orbiting other stars have been giant planets with masses more like Jupiter than Earth, and with orbits located very close to their parent stars. Does this prove that our Solar System is unique? Explain your answer.
- 3. Why are the inner planets made of denser materials than the outer planets?43472445 A 4-9-21 Friday Reading AIXL (4.9.21) D XL| Analyze data to compan A ixl.com/science/grade-8/analyze-data-to-compare-properties-of-planets Test Session Login 6 test.mapnwea.org Use the data to answer the question below. Average distance from the Sun (km) Average orbita (km/s) Planet Mercury 5.79 x 107 47 Venus 1.08 x 10° 35 Earth 1.50 x 10° 30 Mars 2.28 x 108 24 Jupiter 7.79 x 108 13 Saturn 1.43 x 10° 10 Uranus 2.87 x 10° Neptune 4.50 x 10° Is the following statement about our solar system true or false? Mars orbits the Sun at less than 60% of the speed of Earth. true false ATU 5.Which planet or dwarf planet in our solar system has the biggest moon relative to its own size? Not the biggest moon in terms of miles, but biggest compared to the size of the planet it orbits. Jupiter Neptune Uranus Saturn Pluto
- The synchrotron radiation (radio waves) that astronomers first observed from Jupiter in the 1950's comes from a. deep within Jupiter, in the metallic hydrogen layers b. high speed electrons spirling around the planet's strong magnetic field c. the upper-atmosphere clouds that more quickly near the equator of the planet d. the Red Spot with its tremendous friction1. Which of the outer planets have compositions dominated by the "ices" ingredient? Check the correct two. 2. Which of the outer planets have compositions dominated by the "gases" ingredient? Check the correct two. 3. Most of the spaceflight missions to the outer planets have been flyby missions, but two of them were orbiters. Which of these two spacecraft orbited giant planets? Check the correct two. (Hint: An orbiter might do a flyby of one planet and then go on to orbit a different planet.) 4. Jupiter's mass is how many times larger than the Earth's? Just type a number, no words or any other extra stuff. 5. Which of the outer planets has extreme seasons, with its rotational axis being tilted so much that it is practically in the plane of its orbit?20 Approximately how many other planetary systems have been discovered to date? A Tens of thousands B) Tens C Hundreds D Thousands E Millions
- 14. Based on what the nebular theory tells us about the formation of our own solar system, what does the theory predict for the possibility of other planetary systems? Group of answer choices Other planetary systems should be identical to our own. Planetary systems should be very rare. Most stars should have one or two planets, but not more. Planetary systems should be common. 15. Which of the following statements best describes the accomplishments of these three people? Group of answer choices Tycho collected the data, Kepler provided the model in the form of laws, Newton explained the model in terms of gravity. Kepler collected the data, Tycho provided the model in the form of laws, Newton explained the model in terms of gravity. Tycho collected the data, Newton provided the model in the form of laws, Kepler explained the model in terms of gravity. Newton collected the data, Tycho provided the model in the form of laws, Kepler explained the model in terms of gravity.4) Science fiction movies often portray asteroid belts as crowded, dense regions that require spaceships to maneuver quickly to get through them. In this problem, we will calculate the fraction of volume in an asteroid belt that is actually occupied by asteroids. a) If there are 300,000 large asteroids between 2 and 3 AU from the Sun, and each asteroid is assumed to be spherical with a radius of 100 km, determine the total volume occupied by asteroids in this region. Recall that the volume of a sphere is given by the equation V = 4TR³ /3. b) Let's assume the region in which these asteroids orbit is an annulus with an inner radius of 2 AU, an outer radius of 3 AU, and a thickness of 2Ro. Determine the volume of this region. Recall that the area of a circle is given by the equation A = TR². Here are two conversions that you'll need: 1 AU = 1.496 × 108 km and 1 Ro = 6.955 × 105 km. c) What is the ratio of the volume occupied by asteroids to the volume of the asteroid belt (i.e., the…How many orders of magnitude do you need to grow in spatial scale (size) to form a planet? Let's take the extreme ends of this scale, from a dust particle of radius a = 10-6m to the gas giant Jupiter (you can round up its radius to the nearest ten to keep it simple). What else has this difference in order of magnitude? Maybe pick something that's not a length scale. Be creative!