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4,7,8,9,and 10
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The density graph, Figure 4.1d, shows something different. Mercury, Venus, Earth and Mars have
higher densities while the larger, massive planets along with Pluto and Eris all hive lower
densities. The higher densities are because Mercury. Venus, Barth, and Mars are made mostly of
rock and metal while the lower-density objects, Jupiter. Saturn, Uranus, and Neptune, are made
largely of gases and liquids. Being so far from the Sun, Pluto and Eris are composed partly of
ice.4. Based on the comparisons you have made, have any objects been grouped together every
time? How many groups are there?7. Examine the data in Table 4.1 comparing the orbital radius
(distance from the Sun) of each object. Which group is closer to the Sun? Which group is further
from the Sun?8. By now, you may have noticed that there are two major groups of planet
classification. Label each group and list the members of each of your groups: List what properties
from the data table and bar graphs that the objects in each of your groups have in common. 9. Is
(are) there a (any) objects(s) that do not seem to fit into a group? Which objects? Have you heard
about a fairly recent decision made about one of these objects? Did this exercise help clarify the
reason for the decision? 10. State whether or not you agree with each student and why or why not.
Student 1 Pluto and Eris should be in a group with Earth and the other objects like Earth (the
Terrestrial planets) because they are small, of low mass, do not have very many moons, and have
longer rotation periods. Student 2 No, Pluto and Eris should be in a group with Jupiter and the
other objects like lupiter (the Jovian planets) because they have lower density and are far from
Sun. Student 3 Maybe Pluto and Eris do not fit into either category and should be considered a
different type of object than the Ierrestrial or Jovian planets? Small, low mass, lower density
objects with few or no moons and longer rotation periods that are even farther from the Sun than
the Jovian planetsItRIE I 1 Colar Guetom Oiviont Hats Pigure 1.1a, 4.1c, and 4.1d show bar
graphs or histograms comparing the radu fhe mades is the distance from the center of an object to
its edge, a function of its size) of each object listed in Table 4.1. their mass (how much matter
each con. tains) and their density. Density is a combination of mass and size. It is a measure of
how much mass per unit volume an object has. Solids, like rocks and metals, are generally objects
of high density, gases like air, are of low density; and liquids and ices, like water and ice are
usually in between.FlGURE 4.1b Objects 1 to 10 listed in Table 4.1 are shown here from left to
right. Note that the relative distances between these objects are not to scale in this figure. Objects
are shown, from lett to right, in increasing distance lrom the Sun. The mass bar graph, Figure 4.1c
, shows that Jupiter is by far the most massive, then Saturn, with Urams and Neptune the only
others that even register on the graph. Perhaps at this point Jupiter, Saturn. Uranus, and Neptune
could be considered a group of large and massive planets while Earth and all the others could be
called small and less massive planets.

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SURVEY I created for uni project research
SURVEY I created for uni project researchSURVEY I created for uni project research
SURVEY I created for uni project research
 

need help with questions 4789and 10 Ill rate thank yo.pdf

  • 1. need help with questions 4,7,8,9,and 10 I'll rate. thank you The density graph, Figure 4.1d, shows something different. Mercury, Venus, Earth and Mars have higher densities while the larger, massive planets along with Pluto and Eris all hive lower densities. The higher densities are because Mercury. Venus, Barth, and Mars are made mostly of rock and metal while the lower-density objects, Jupiter. Saturn, Uranus, and Neptune, are made largely of gases and liquids. Being so far from the Sun, Pluto and Eris are composed partly of ice.4. Based on the comparisons you have made, have any objects been grouped together every time? How many groups are there?7. Examine the data in Table 4.1 comparing the orbital radius (distance from the Sun) of each object. Which group is closer to the Sun? Which group is further from the Sun?8. By now, you may have noticed that there are two major groups of planet classification. Label each group and list the members of each of your groups: List what properties from the data table and bar graphs that the objects in each of your groups have in common. 9. Is (are) there a (any) objects(s) that do not seem to fit into a group? Which objects? Have you heard about a fairly recent decision made about one of these objects? Did this exercise help clarify the reason for the decision? 10. State whether or not you agree with each student and why or why not. Student 1 Pluto and Eris should be in a group with Earth and the other objects like Earth (the Terrestrial planets) because they are small, of low mass, do not have very many moons, and have longer rotation periods. Student 2 No, Pluto and Eris should be in a group with Jupiter and the other objects like lupiter (the Jovian planets) because they have lower density and are far from Sun. Student 3 Maybe Pluto and Eris do not fit into either category and should be considered a different type of object than the Ierrestrial or Jovian planets? Small, low mass, lower density objects with few or no moons and longer rotation periods that are even farther from the Sun than the Jovian planetsItRIE I 1 Colar Guetom Oiviont Hats Pigure 1.1a, 4.1c, and 4.1d show bar graphs or histograms comparing the radu fhe mades is the distance from the center of an object to its edge, a function of its size) of each object listed in Table 4.1. their mass (how much matter each con. tains) and their density. Density is a combination of mass and size. It is a measure of how much mass per unit volume an object has. Solids, like rocks and metals, are generally objects of high density, gases like air, are of low density; and liquids and ices, like water and ice are usually in between.FlGURE 4.1b Objects 1 to 10 listed in Table 4.1 are shown here from left to right. Note that the relative distances between these objects are not to scale in this figure. Objects are shown, from lett to right, in increasing distance lrom the Sun. The mass bar graph, Figure 4.1c , shows that Jupiter is by far the most massive, then Saturn, with Urams and Neptune the only others that even register on the graph. Perhaps at this point Jupiter, Saturn. Uranus, and Neptune could be considered a group of large and massive planets while Earth and all the others could be called small and less massive planets.