Science: Cosmic dance dust holds clues to origin of life
Near-Infrared image (NACO/VLT) of V1280 Sco. (Chesneau et al., Astronomy & Astrophysics, 2012) (PIB)
By Our Special Correspondent
New Delhi, August 23: In the winter of 2007, astrophysicists from all over the world made a beeline to observatories on mountaintops to observe a bright explosion born out of the cosmic dance of a white dwarf and its companion star, resulting in thick dust around an imploding novae.
Dr RK Das, a scientist from SN Bose Centre for Basic Science (SNBCBS), stationed himself at Mount Abu Observatory.
His team observed the imploding novae called Nova V1280 Scorpii and found that a thick dust formed around it after a month and lasted for about 250 days.
The team from SNBCBS, an autonomous institute of Department of Science and Technology (DST), used the observed data on infrared spectra of the imploding novae and constructed simple models which helped them estimate its parameters like hydrogen density, temperature, luminosity and elemental abundances during pre- and post-dust phase.
“They have found high abundance of certain elements like carbon, nitrogen and oxygen in the ejecta along with a mixture of small amorphous carbon dust grains and large astrophysical silicate dust grains,” said the Ministry of Science and technology.
The dust formation was observed in parallel by international collaborators of the team from the ‘Very Large Telescope Interferometer’ in Chile.
This helped them take precision measurements of the rate of the expansion of the dust shell around a nova for the first time.
“The stellar event which was golden opportunity for scientists to study the exploding stellar matter was an example of space-dust collisions which could propel organisms over enormous distances between planets to start life on a planet,” added the ministry.
The study of novae dust could help in understanding the nature and characteristics of the dust and associated processes.
“Cosmic dust or extra-terrestrial dust formation in the hostile environment of novae ejection has been an open question for many years. Hundreds of kilograms of such dust fall on the Earth every day. However, formation, nature and composition of the dust are not properly understood yet,” said the ministry on the outcome of the research.
“Dust formation in novae ejecta is not a common phenomenon. It has been observed only in a few novae within 30 to 100 days after an outburst, as compared to interstellar dust, which typically takes a few thousand years to form and hence provided opportunity to study the dust formation process in novae,’ Dr. Das explained.
The team varied the parameters over a wide range and constructed more than 50,000 models generating spectrum for each model.
Finally, they fit the observed spectrum with the model generated ones.
From the best fit, they estimated the parameters during pre- and post-dust phase.
“Such a detailed modelling of a dust forming Nova had never been done before. The entire process took a couple of years,” added the ministry.
Besides high abundance of certain elements like carbon, nitrogen and oxygen in pre-dust phase of the imploding novae as compared to solar values, the scientists found a mixture of small amorphous carbon dust grains and large astrophysical silicate dust grains present in the ejecta in the post-dust phase.
Some complex organic compounds like amorphous organic solids with a mixed aromatic–aliphatic structure were found which play an important role in formation of molecular cloud in stars and planets.
The study was published in the journal Astrophysical Journal recently.
The team has suggested that as the expanding dust shell of V1280 Scorpii Nova continued to expand these dust grains will eventually mix with interstellar matter.
But that will take thousands of years – a small time in the cosmic time scale.
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