DK Eyewitness - Astronomy
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Wood<br />
Looking at volume<br />
These blocks—wood, aluminum, and iron—all have<br />
the same volume, that is they occupy the same amount<br />
of space. Despite being the same size, however, these<br />
materials do not have the same mass and density, nor do<br />
they weigh the same. This is also true of the planets.<br />
For example, Mercury, though small, has a higher<br />
density than that of some of the larger planets.<br />
Wood<br />
Aluminum<br />
Iron<br />
Measuring planets<br />
Whereas we can weigh and<br />
measure objects on Earth, we<br />
have to assess the space a planet<br />
occupies (volume), how much<br />
matter it contains (mass), and its<br />
density by looking at its behavior,<br />
by analyzing its gravitational pull<br />
on nearby objects, and by using<br />
data gained by space probes<br />
(pp.34–35). Density is the mass for<br />
every unit of volume of an object<br />
(mass divided by the volume).<br />
Measuring mass<br />
Mass is how much matter an object contains.<br />
A beam balance can be used to find the mass of a<br />
Mercury<br />
material. Here a piece of wood and a piece of iron of<br />
identical proportions and volume are placed on the<br />
balance. The iron has the greater mass. By dividing the<br />
Orbital period<br />
mass (measured in grams) of the wood and the iron<br />
The tidal force of Earth has locked<br />
by their volume (measured in cubic centimeters), their<br />
its Moon into rotating so that one<br />
relative densities can be calculated.<br />
side of the Moon always faces Earth<br />
(p.40). This means the rotational period<br />
of the Moon equals its monthly period of<br />
revolution around Earth. Since the orbit of<br />
Mercury is elongated, like an oval, it is locked<br />
into a rotational period where the planet<br />
spins 1½ times during each orbit of the Sun.<br />
This means that its year (how long it takes to<br />
orbit the Sun) is 88 Earth days, while its day<br />
(the time it takes to rotate—sunrise to<br />
sunrise) is 58.6 Earth days.<br />
Iron<br />
Saturn<br />
Comparing density<br />
Mercury has great mass for its size. Even<br />
though it is only slightly larger than Earth’s<br />
Moon, its mass is four times that of the Moon.<br />
This means its density must be nearly as<br />
high as Earth’s, most likely due to a very high<br />
quantity of iron. Astronomers believe that<br />
Mercury must have a massive iron core that<br />
takes up nearly three-fourths of its radius to<br />
achieve such great mass—a fact backed up<br />
by Mariner 10’s evidence of a magnetic field.<br />
When the densities of Mercury and Saturn,<br />
the huge gas giant (pp.52–53), are compared,<br />
Saturn would float and Mercury, whose<br />
density is seven times as great, would sink.<br />
Moon Earth Mercury<br />
Crater<br />
Facts about mercury<br />
Mosaic of<br />
separate<br />
photographs<br />
Rocky crust<br />
Iron and<br />
nickel core<br />
Rocky mantle<br />
• Sidereal period 88 Earth days<br />
• Temperature at surface –292°F to 800°F (−180°C to 430°C)<br />
• Rotational period 58.6 Earth days<br />
• Mean distance from the Sun 36 million miles/<br />
57.9 million km<br />
• Volume (Earth = 1) 0.056 • Mass (Earth = 1) 0.055<br />
• Density (water = 1) 5.43<br />
• Equatorial diameter 4,879 km/3,030 miles<br />
• Number of satellites 0