Meetings on Comets & Meeting Comet People!

Many solar system researchers met at the IAU Commission F1 Meteoroids 2016 at ESA/ESTEC, Noordwijk, Netherlands and Cometary Science After Rosetta Meeting 2016 at the Royal Society, London, England, both held in Jun 2016. CEED postdoc Aswin Sekhar was one of the participants for both conferences and presented the latest results representing the CEED Earth & Beyond Team. The primary aims of both these meetings were to enhance the studies of solar system small bodies and bring together researchers from different fields of astrophysics and geophysics communities to extend further collaborations.

Photo 1. Image of 67P/Churyumov-Gerasimenko nuclei (Credits: ESA/Rosetta team)

Text by: Dr. Aswin Sekhar (postdoc at CEED)

Comets have always fascinated scientists as well as the general public
since time immemorial. Once upon a time, comets were considered as
‘carriers of bad omen’ and hence special interest went into studying and
predicting their arrival in ancient civilisations. There are various
references in history related to rituals and ceremonies conducted by old
civilisations (evidence found in Mayan records by archae-astronomers was
discussed in this conference too) in conjunction with appearances of
comets and meteor showers.

After the invention of telescopes, it was possible to observe these objects
with better clarity and find reasonably accurate astrometric positions
so that their orbital details could be gathered. These orbital
parameters, compiled from repeated observations, enabled scientists to
predict the past and future of cometary orbits using Newton’s equations
of motion and various other standard techniques in celestial mechanics.

Photo 2. Excitingly, the venue of this meeting on comets had the original telescope (presented by Newton himself to the Royal Society in 1671) preserved and open as an exhibit for the meeting attendees.
















Inspite of the outstanding contributions and wealth of knowledge
acquired from the ‘formative’ comet era extending from Halley to
Whipple, our studies about these bodies restricted to measurements from
a large distance (using telescopes). But cometary science has matured
drastically since then.

In 1986, European Space Agency’s (ESA) Giotto mission had a close flyby
to comet 1P/Halley during its most recent journey near the sun. This was
a significant step ahead of all the previous ground based telescope
observations of comets.

The studies on comets took an unprecedented new level in 2014 by the
successful ESA’s Rosetta mission sending a lander Philae on to the
surface of a comet (for more background on the mission, check Stephanie
Werner’s previous article:
The final chosen destination for this mission was the comet

Photo 3. Meeting with the co-discoverer (Dr Churyumov) of the Rosetta mission target comet 67P/Churyumov-Gerasimenko from ESA/ESTEC.












During both these conferences, there were various interesting ideas
regarding the formation and future of 67P, which has earned the nickname
as a ’rubber duck comet’. There were multiple schools of thoughts
regarding two or more separate pieces of material clumping together to
form the ‘rubber duck shape’ which we see clearly from observations (see
photo 1). Few scientists speculate the comet fragmenting into two due
to the strong outgassing at the ‘neck’ feature (see photo 1) and
leading it to become a binary comet system in future.

Because 67P is rocky and icy at the same time, there were interesting
debates about the boundaries between the classification of asteroids and
comets. Because there are new asteroids which are being found comet-like
(i.e. actively outgassing or ejecting material) and new comets being
found which are asteroid-like (i.e. rocky or metallic), most of the
community tend to agree that there is an asteroid-comet continuum in our
solar system rather than two discrete populations strictly separated
from each other (as previously thought).

Few discussions focused on the unique sungrazing cometary population
which come dangerously close to the sun such that some of them get
either fragmented (due to tidal forces from the sun) or evaporate (due
to solar heat) or fall into the sun (due to near sun colliding orbits by
Kozai mechanism). Interesting theories were presented about the
formation, influx and long term dynamical evolution of Jupiter family
(orbital period upto 20 years) and Halley-type comets (orbital period
from 20 to 200 years) from their source regions like the Kuiper belt and
the Oort cloud.

In connection to the bigger picture, new results were presented by
different scientists regarding the impact risks on Earth from different
small body populations like fireballs, bolides, asteroids and comets.
The latest calibrated frequency vs impactor size estimates were
presented and discussed using observational records compiled over last
couple of decades.

For the safety of future space and satellite missions and to prevent
them from high velocity meteoroid impacts, new approaches of modelling
of dust trails in the neighbourhood of spacecraft was envisaged. For a
short animation (developed by Dr Rachel Soja, Institute of Space
Systems, University of Stuttgart) of the dynamical evolution of ejected
dust trails from comet 67P (i.e. Rosetta mission target), check the

Both these conferences generated a good scientific and social overlap
between the theoreticians, professional observers, amateur observers and
space educators. Although scientists generally tend to disagree
(peacefully?!) with each other about most things in life, on a
lighter note, I think everyone jointly agreed on the famous Levy’s
quote: “comets are like cats; they have tails, and they do precisely
what they want!’” 

Published July 7, 2016 11:40 AM - Last modified July 7, 2016 11:40 AM