Robert M. Hazen

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Robert M. Hazen


Born
in Rockville Centre, NY , The United States
November 01, 1948

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Robert M. Hazen, Senior Research Scientist at the Carnegie Institution of Washington’s Geophysical Laboratory and the Clarence Robinson Professor of Earth Science at George Mason University, received the B.S. and S.M. in geology at the Massachusetts Institute of Technology (1971), and the Ph.D. at Harvard University in earth science (1975). The Past President of the Mineralogical Society of America, Hazen’s recent research focuses on the possible roles of minerals in the origin of life. He is also Principal Investigator of the Deep Carbon Observatory.

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Quotes by Robert M. Hazen  (?)
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“The lessons of rocks, stars,and life are clear. To understand Earth, you must divorce yourself for the inconsequential temporal or spacial scale of human life. We live on a single tiny world in a cosmos of a hundred billion galaxies, each with a hundred billion stars. Similarly, we live day by day in a cosmos aged hundreds of billions of days. If you seek meaning and purpose in the cosmos, you will not find it in any privileged moment or place tied to human existence.”
Robert m hazen, The Story of Earth: The First 4.5 Billion Years, from Stardust to Living Planet

“To get a sense of the scale of Earth history, imagine walking back in time, a hundred years per step—every pace equal to more than three human generations. A mile takes you 175,000 years into the past. The twenty miles of Chesapeake cliffs, a hard day’s walk to be sure, correspond to more than 3 million years. But to make even a small dent in Earth history, you would have to keep walking at that rate for many weeks. Twenty days of effort at twenty miles a day and a hundred years per step would take you back 70 million years, to just before the mass death of the dinosaurs. Five months of twenty-mile walks would correspond to more than 530 million years, the time of the Cambrian “explosion”—the near-simultaneous emergence of myriad hard-shelled animals. But at a hundred years per footstep, you’d have to walk for almost three years to reach the dawn of life, and almost four years to arrive at Earth’s beginnings.”
Robert M. Hazen, The Story of Earth: The First 4.5 Billion Years, from Stardust to Living Planet

“No direct evidence yet documents Earth’s tidal cycles more than a billion years ago, but we can be confident that 4.5 billion years ago things were a lot wilder. Not only did Earth have five-hour days, but the nearby Moon was much, much faster in its close orbit, as well. The Moon took only eighty-four hours—three and a half modern days—to go around Earth. With Earth spinning so fast and the Moon orbiting so fast, the familiar cycle of new Moon, waxing Moon, full Moon, and waning Moon played out in frenetic fast-forward: every few five-hour days saw a new lunar phase. Lots of consequences follow from this truth, some less benign than others. With such a big lunar obstruction in the sky and such rapid orbital motions, eclipses would have been frequent events. A total solar eclipse would have occurred every eighty-four hours at virtually every new Moon, when the Moon was positioned between Earth and the Sun. For some few minutes, sunlight would have been completely blocked, while the stars and planets suddenly popped out against a black sky, and the Moon’s fiery volcanoes and magma oceans stood out starkly red against the black lunar disk. Total lunar eclipses occurred regularly as well, almost every forty-two hours later, like clockwork. During every full Moon, when Earth lies right between the Sun and the Moon, Earth’s big shadow would have completely obscured the giant face of the bright shining Moon. Once again the stars and planets would have suddenly popped out against a black sky, as the Moon’s volcanoes put on their ruddy show. Monster tides were a far more violent consequence of the Moon’s initial proximity. Had both Earth and the Moon been perfectly rigid solid bodies, they would appear today much as they did 4.5 billion years ago: 15,000 miles apart with rapid rotational and orbital motions and frequent eclipses. But Earth and the Moon are not rigid. Their rocks can flex and bend; especially when molten, they swell and recede with the tides. The young Moon, at a distance of 15,000 miles, exerted tremendous tidal forces on Earth’s rocks, even as Earth exerted an equal and opposite gravitational force on the largely molten lunar landscape. It’s difficult to imagine the immense magma tides that resulted. Every few hours Earth’s largely molten rocky surface may have bulged a mile or more outward toward the Moon, generating tremendous internal friction, adding more heat and thus keeping the surface molten far longer than on an isolated planet. And Earth’s gravity returned the favor, bulging the Earth-facing side of the Moon outward, deforming our satellite out of perfect roundness.”
Robert Hazen, The Story of Earth: The First 4.5 Billion Years, from Stardust to Living Planet

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