#5. My favourite celestial body, Earth’s moon. For... - Wissenschaft und Deutsch

#5. My favourite celestial body, Earth’s moon. For some reason I’ve been obsessed with it, even as a child, when I first asked my mom to buy me a telescope. 

Our Moon makes Earth a more livable planet by moderating our home planet’s wobble on its axis, leading to a relatively stable climate, and creating a rhythm that has guided humans for thousands of years. The Moon was likely formed after a Mars-sized body collided with Earth and the debris formed into the most prominent feature in our night sky.

The regular daily and monthly rhythms of Earth’s only natural satellite, the Moon, have guided timekeepers for thousands of years. Its influence on Earth’s cycles, notably tides, has been charted by many cultures in many ages. Color illustration shows ice concentrations in a lunar crater. Ice may make up as much as 22% of the surface material in Shackleton crater. Color image of astronaut next to giant moon boulder. An astronaut next to a huge, split boulder on the moon. Black and white of lunar crater. Rugged Copernicus crater. The presence of the Moon moderates Earth’s wobble on its axis, leading to a relatively stable climate over billions of years. From Earth, we always see the same face of the Moon because the Moon rotates once on its own axis in the same time that it travels once around Earth (called synchronous rotation). The light areas of the Moon are known as the highlands. The dark features, called maria (Latin for seas), are impact basins that were filled with lava between 4 and 2.5 billion years ago. Though the Moon has no internally generated magnetic field, areas of magnetism are preserved in the lunar crust, but how this occurred is a mystery. The early Moon appears not to have had the right conditions to develop an internal dynamo, the mechanism for global magnetic fields for the terrestrial planets. How did the Moon come to be? The leading theory is that a Mars-sized body collided with Earth approximately 4.5 billion years ago, and the resulting debris from both Earth and the impactor accumulated to form our natural satellite. The newly formed Moon was in a molten state. Within about 100 million years, most of the global “magma ocean” had crystallized, with less dense rocks floating upward and eventually forming the lunar crust. With essentially no atmosphere to impede impacts, a steady rain of asteroids, meteoroids and comets strike the surface. Over billions of years, the surface has been ground up into fragments ranging from huge boulders to powder. Nearly the entire Moon is covered by a rubble pile of charcoal-gray, powdery dust and rocky debris called the lunar regolith. Beneath the regolith is a region of fractured bedrock referred to as the megaregolith. Four impact structures are used to date objects on the Moon: the Nectaris and Imbrium basins and the craters Eratosthenes and Copernicus. Lunar history is based on time segments bounded by the age of each impact structure. A Copernican feature, for example, is as young or younger than the impact crater Copernicus, that is, about one billion years old or less. The Moon was first visited by the USSR’s Luna 1 and Luna 2 in 1959. These were followed by a number of U.S. and Soviet robotic spacecraft. The U.S. sent three classes of robotic missions to prepare the way for human exploration: the Rangers (1961-1965) were impact probes, the Lunar Orbiters (1966-1967) mapped the surface to find landing sites and the Surveyors (1966-1968) were soft landers. The first human landing on the Moon was on 20 July 1969. During the Apollo missions of 1969-1972, 12 American astronauts walked on the Moon and used a Lunar Roving Vehicle to travel on the surface and extend their studies of soil mechanics, meteoroids, lunar ranging, magnetic fields and solar wind. The Apollo astronauts brought back 382 kg (842 pounds) of rock and soil to Earth for study. After a long hiatus, lunar exploration resumed in the 1990s with the U.S. robotic missions Clementine and Lunar Propspector. Results from both missions suggest that water ice may be present at the lunar poles, but a controlled impact of the Prospector spacecraft produced no observable water. A new era of international lunar exploration began in earnest in the new millennium. The European Space Agency was first with SMART-1 in 2003, followed by three spacecraft from other nations during the years 2007 and 2008: Kaguya (Japan), Chang’e-1 (China), and Chandrayaan-1 (India). The U.S. began a new series of robotic lunar missions with the joint launch of the Lunar Reconnaissance Orbiter and LCROSS in 2009. More missions are planned in anticipation of sending human beings back to the Moon.

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