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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

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