Proof that Comets Brought Oceans to Earth
Observations of Hartley 2 have revealed the first comet with water similar to that on our home planet
Even though it sounds like a paradox, water is an immigrant on our blue planet. In the early days of our planetary system, Earth was so hot that all volatiles such as water evaporated. Only the outer regions of our solar system beyond the orbit of Mars remained rich in water. From there, it is believed to have returned to Earth approximately 3.9 billion years ago -- “on board” asteroids, as scientists have assumed until now.
“Current theories came to the result that less than ten percent of Earth’s water originated from comets”, Dr. Paul Hartogh from MPS, who led the new study, explains. “Now for the first time, our results imply that comets may have played a much more important role”, Dr. Miriam Rengel from MPS adds.
Until now, this held true mainly for asteroids from the outer rim of the so-called asteroid belt close to Jupiter’s orbit. The six comets for which conclusions concerning this ratio have been possible so far are likely much richer in deuterium. All these comets are believed to have originated in the vicinity of the large gas planets Jupiter, Saturn, Uranus, and Neptune.
Hartley 2, however, is different. Scientists believe that its cosmic home lies in the Kuiper belt, a region on the outer limits of our solar system. In October and November 2010, Hartley 2 passed Earth as closely as never before since its discovery. During this encounter, also the instruments on board the space observatory Herschel were therefore aimed at the comet. With the help of exact observations of its coma -- the sheath of gas and dust surrounding comets when they come close to the Sun -- the researchers hoped to determine the deuterium-to-hydrogen ratio.
“The water molecules within the coma emit a characteristic radiation in the far infrared”, says Hartogh. This also holds true for the heavier cousin of water: water molecules in which one hydrogen atom has been replaced by a deuterium atom. “From this characteristic radiation we can determine the ratio of deuterium to hydrogen”, he adds. However, since the heavy water is very rare, its radiation intensity is extremely weak. Nevertheless, with Herschel’s HIFI instrument, the most sensitive detector for water vapor, the researchers were able to detect the molecule with an astonishingly good signal-to-noise ratio.
Determining where Earth's water came from is important for astrobiologists because its a key peice in the puzzle of how Earth became habitable for life.
However, the new results also raise new questions. Until now, scientists assumed that the distance of a body’s origin from the Sun correlated to the deuterium-to-hydrogen ratio in its water. The farther away this origin lies from the Sun, the larger this ratio should be. With a “birth place” within the Kuiper belt and thus well beyond the orbit of Neptune, Hartley 2, however, seems to violate this rule. “Either the comet originated in greater proximity to the Sun than we thought”, says Hartogh, “or the current assumptions on the distribution of deuterium have to be reconsidered.” And maybe Hartley 2 is a so-called Trojan that originated close to Jupiter and could never overcome its gravitational pull.