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— CH. 1 · DISCOVERY AND NAMING HISTORY —

67P/Churyumov–Gerasimenko

~5 min read · Ch. 1 of 6
6 sections
  • On the 11th of September 1969, a photographic plate exposed at the Alma-Ata Astrophysical Institute captured a faint smudge near the edge of the frame. Klim Ivanovich Churyumov examined this image while working at Kyiv University's Astronomical Observatory. He initially assumed the object was comet Comas Solà because it appeared in that region of the sky. After returning to his home institute, he scrutinized all available plates from the observatory. On the 22nd of October, about one month after the exposure, Churyumov realized the object could not be Comas Sol'. It sat approximately 1.8 degrees off its expected position. Further analysis revealed a faint image of Comas Sol' at its correct location on the same plate. This proved the other object was a distinct body. Svetlana Ivanovna Gerasimenko had taken the original photograph during her shift. The pair named the new discovery after themselves, creating the designation 67P/Churyumov, Gerasimenko.

  • The nucleus measures roughly four kilometers across its longest dimension and two kilometers wide. A smaller lobe connects to a larger one via a narrow neck structure. Scientists determined this shape resulted from a gentle collision between two separate objects moving at low velocity. Each orbit strips away matter as gas and dust evaporate under solar heat. By 2015, estimates suggested a layer averaging three meters thick disappeared per revolution. The total mass reached approximately ten billion tonnes. Rosetta instruments detected sixteen organic compounds within the ice and dust. Four of these substances appeared for the first time on any comet. These included acetamide, acetone, methyl isocyanate, and propionaldehyde. Glycine stood out as the only amino acid found so far. Solid carbon bound itself into very large macromolecular compounds similar to meteoritic material. Free molecular oxygen surrounded the comet in quantities never before seen in cometary comas. This finding challenged existing models suggesting such oxygen should have reacted long ago. Measurements indicated the ratio remained isotropic throughout the coma regardless of distance from the sun.

  • This Jupiter-family comet likely originated in the Kuiper belt before being ejected toward the inner Solar System. Encounters with Jupiter successively altered its path over millions of years. On the 4th of February 1959, a close approach moved the perihelion inward significantly. That interaction set the current trajectory where it remains today. Before the 2009 passage, the rotational period lasted 12.76 hours. During that same year, sublimation-induced torque shortened the spin to 12.4 hours. Future encounters will continue changing the orbit until the object either collides with a planet or escapes entirely. In November 2220, the comet will pass about 0.8 astronomical units from Jupiter again. This event will push the perihelion even closer to the Sun. The orbit stretches from just inside Mars' path to beyond Jupiter's reach. Perihelion distances vary across epochs ranging from 0.8 AU to nearly 3 AU depending on gravitational interactions. These shifts demonstrate how planetary gravity shapes cometary evolution over deep time.

  • European Space Agency launched the Rosetta spacecraft on the 2nd of March 2004. Ground controllers reduced relative velocity by several meters per second using thruster firings starting in May 2014. They successfully rendezvoused with Churyumov, Gerasimenko on the 6th of August 2014. The orbiter entered orbit around the nucleus on the 10th of September at roughly 100 kilometers distance. Hubble Space Telescope images taken on the 12th of March 2003 provided early preparation data for the mission. Detailed observations later came from the Faulkes Telescope on the 25th of April 2012 during aphelion. Water vapor release rates reached approximately one kilogram per second when Rosetta was close to the comet. Images captured on the 14th of July 2014 confirmed the irregular two-lobed shape of the nucleus. By September 2015, scientists concluded the contact binary hypothesis was correct beyond doubt. The mission ended on the 30th of September 2016 when Rosetta landed in the Ma'at region. This final controlled impact marked the conclusion of a twelve-year journey through space.

  • Descent occurred on the 12th of November 2014 as Philae touched down on the Agilkia landing site. Gravity measured only about ten to the minus three meters per second squared. Landing gear deployed but failed to anchor properly due to low gravity conditions. Cold gas thrusters and harpoons did not operate as planned. Ice screws mounted on legs could not gain purchase on the surface. The probe bounced twice before coming to rest after its third contact with the ground. Contact was lost on the 15th of November 2014 because battery power dropped below operational levels. Communications briefly resumed on the 14th of June 2015 showing a healthy spacecraft state. On the 2nd of September 2016, photographs taken by the orbiter located Philae inside a crack. Only the body and two legs remained visible above the debris. This discovery allowed scientists to contextualize data returned from the comet's surface. The lander had traveled roughly 38 million miles during its approach phase.

  • Many geological changes appeared on the surface during Rosetta's lifetime near perihelion. Circular patterns in smooth terrains grew several meters wide each day over time. A fracture within the neck region expanded significantly while boulders tens of meters across shifted positions. Some rocks traveled more than 100 meters away from their original locations. Patches of ground disappeared entirely exposing new features beneath them. Collapsing cliffs became frequent events recorded throughout the mission duration. One notable example occurred in December 2015 when Rosetta NAVCAM captured a bright light patch. Scientists identified this as a large cliff collapse causing an outburst of activity. An apparent outburst observed on the 14th of November 2021 happened while the comet was 1.23 astronomical units from the Sun. Dust mass increased substantially during these events with effective geometric cross-section growing by twenty-seven percent. Two distinct outbursts marked the 2021 apparition period showing varying intensities. Active pits related to sinkhole collapses also appeared regularly on the surface.

Common questions

Who discovered 67P/Churyumov, Gerasimenko and when was it first photographed?

Klim Ivanovich Churyumov and Svetlana Ivanovna Gerasimenko discovered the comet after a photographic plate exposed on the 11th of September 1969 captured a faint smudge near the edge of the frame. They named the new discovery 67P/Churyumov, Gerasimenko following their analysis at Kyiv University's Astronomical Observatory.

What is the physical structure and composition of 67P/Churyumov, Gerasimenko nucleus?

The nucleus measures roughly four kilometers across its longest dimension and two kilometers wide with a smaller lobe connecting to a larger one via a narrow neck structure. Scientists detected sixteen organic compounds within the ice and dust including acetamide, acetone, methyl isocyanate, propionaldehyde, and glycine as the only amino acid found so far.

How did Jupiter influence the orbit of 67P/Churyumov, Gerasimenko over time?

Encounters with Jupiter successively altered the path of this Jupiter-family comet before moving the perihelion inward significantly on the 4th of February 1959. Future encounters will continue changing the orbit until the object either collides with a planet or escapes entirely.

When did the European Space Agency launch Rosetta and when did it land on 67P/Churyumov, Gerasimenko?

European Space Agency launched the Rosetta spacecraft on the 2nd of March 2004 and successfully rendezvoused with Churyumov, Gerasimenko on the 6th of August 2014. The mission ended on the 30th of September 2016 when Rosetta landed in the Ma'at region after entering orbit around the nucleus on the 10th of September at roughly 100 kilometers distance.

What happened to the Philae lander during its descent on 67P/Churyumov, Gerasimenko?

Descent occurred on the 12th of November 2014 as Philae touched down on the Agilkia landing site but bounced twice before coming to rest after its third contact with the ground due to low gravity conditions. Contact was lost on the 15th of November 2014 because battery power dropped below operational levels and photographs taken by the orbiter located Philae inside a crack on the 2nd of September 2016.

All sources

106 references cited across the entry

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