THE MOON
GENERAL INFORMATION
The Moon (or Luna) is the Earth’s only natural satellite and was formed 4.6 billion years ago around some 30–50 million years after the formation of the solar system. The Moon is in synchronous rotation with Earth meaning the same side is always facing
the Earth. The first unmanned mission to the Moon was in 1959 by the Soviet Lunar Program with the first manned landing being Apollo 11 in 1969.
PROFILE
- Circumference at Equator: 10,917.0 km
- Diameter: 3,475 km
- Mass: 73,476,730,924,573,500 million kg (0.0123 x Earth)
- Orbits: The Earth
- Average Distance from Earth: 384,400 km
- Length of Orbit: 27.3 Earth days
- Surface Temperature: -233 to 123 °C
THE DARK SIDE OF THE MOON
In reality both sides of the Moon see the same amount of sunlight however only one face of the Moon is ever seen from Earth. This is because the Moon rotates around on its own axis in exactly the same time it takes to orbit the Earth, meaning the same
side is always facing the Earth. The side facing away from Earth has only been seen by the human eye from spacecraft.
THE RISE AND FALL OF THE TIDES ARE CAUSED BY THE MOON
There are two bulges in the Earth due to the gravitational pull that the Moon exerts; one on the side facing the Moon, and the other on the opposite side that faces away from the Moon, The bulges move around the oceans as the Earth rotates, causing high
and low tides around the globe.
THE MOON IS DRIFTING AWAY FROM THE EARTH
The Moon is moving approximately 3.8 cm away from our planet every year. It is estimated that it will continue to do so for around 50 billion years. By the time that happens, the Moon will be taking around 47 days to orbit the Earth instead of the current
27.3 days.
A PERSON WOULD WEIGH MUCH LESS ON THE MOON
A person would weigh much less on the Moon: The Moon has much weaker gravity than Earth, due to its smaller mass, so you would weigh about one sixth (16.5%) of your weight on Earth. This is why the lunar astronauts could leap and bound so high in the air.
EARTH
General Information
Earth is the third planet from the Sun and is the largest of the terrestrial planets. The Earth is the only planet in our solar system not to be named after a Greek or Roman deity. The Earth was formed approximately 4.54 billion years ago and is the only known planet to support life.
Profile
- Mass: 5,972,190,000,000,000 billion kg
- Equatorial Diameter: 12,756 km
- Polar Diameter: 12,714 km
- Equatorial Circumference: 40,030 km
- Known Moons: 1
- Notable Moons: The Moon
- Orbit Distance: 149,598,262 km (1 AU)
- Orbit Period: 365.26 Earth days
- Surface Temperature: -88 to 58°C
The Earth’s rotation is gradually slowing
This deceleration is happening almost imperceptibly, at approximately 17 milliseconds per hundred years, although the rate at which it occurs is not perfectly uniform. This has the effect of lengthening our days, but it happens so slowly that it could be as much as 140 million years before the length of a day will have increased to 25 hours.
The Earth was once believed to be the centre of the universe
Due to the apparent movements of the Sun and planets in relation to their viewpoint, ancient scientists insisted that the Earth remained static, whilst other celestial bodies travelled in circular orbits around it. Eventually, the view that the Sun was at the centre of the universe was postulated by Copernicus, though this is also not the case.
Earth has a powerful magnetic field
This phenomenon is caused by the nickel-iron core of the planet, coupled with its rapid rotation. This field protects the Earth from the effects of solar wind.
There is only one natural satellite of the planet Earth
As a percentage of the size of the body it orbits, the Moon is the largest satellite of any planet in our solar system. In real terms, however, it is only the fifth largest natural satellite.
Earth is the only planet not named after a god
The other seven planets in our solar system are all named after Roman gods or goddesses. Although only Mercury, Venus, Mars, Jupiter and Saturn were named during ancient times, because they were visible to the naked eye, the Roman method of naming planets was retained after the discovery of Uranus and Neptune.