Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

Unusual polarimetric properties for interstellar comet 2I/Borisov

View through CrossRef
<p><strong>Introduction</strong></p> <p>Only two interstellar objects have been observed passing through our Solar System to date. The first one, 1I/‘Oumuamua, discovered in 2017 in its post-perihelion phase, showed mostly asteroidal characteristics with some potential evidence of comet-like behaviour, but 2I/Borisov has showed clear evidence of comet activity since its discovery in 2019, prior to its perihelion passage in December of that year. This made it the first confirmed interstellar comet, so naturally many different observations were conducted by astronomers around the world to learn more about the peculiar object.</p> <p><strong>Methodology</strong></p> <p>In this work we present the analysis of polarimetric observations of the interstellar comet 2I/Borisov conducted with the FORS2 instrument located on the European Southern Observatory's Very Large Telescope Unit 1 (Antu). A series of polarimetric observations was performed between December 2019 and March 2020 using three different broadband filters in the visible regime in order to ascertain the physical characteristics of the coma dust particles.</p> <p><strong>Results & Conclusions</strong></p> <p>We find that polarisation of 2I/Borisov is higher than is usually measured for Solar System comets. This distinguishes the interstellar comet from all dynamically evolved comets in our Solar System. This evidence of 2I/Borisov being more pristine than the observed Solar System comets is corroborated by the fact that the comet with the closest polarimetric properties is C/1995 O1 (Hale–Bopp), which is believed to have approached the Sun only once before its apparition in 1997. Furthermore, and unlike both Hale–Bopp and many other comets, interstellar comet 2I/Borisov shows a polarimetrically homogeneous coma, unchanging with cometocentric distance, again suggesting it is even more pristine than the observed comets from our own Solar System. It is thus likely that it has never passed very close to its native star.</p>
Title: Unusual polarimetric properties for interstellar comet 2I/Borisov
Description:
<p><strong>Introduction</strong></p> <p>Only two interstellar objects have been observed passing through our Solar System to date.
The first one, 1I/‘Oumuamua, discovered in 2017 in its post-perihelion phase, showed mostly asteroidal characteristics with some potential evidence of comet-like behaviour, but 2I/Borisov has showed clear evidence of comet activity since its discovery in 2019, prior to its perihelion passage in December of that year.
This made it the first confirmed interstellar comet, so naturally many different observations were conducted by astronomers around the world to learn more about the peculiar object.
</p> <p><strong>Methodology</strong></p> <p>In this work we present the analysis of polarimetric observations of the interstellar comet 2I/Borisov conducted with the FORS2 instrument located on the European Southern Observatory's Very Large Telescope Unit 1 (Antu).
A series of polarimetric observations was performed between December 2019 and March 2020 using three different broadband filters in the visible regime in order to ascertain the physical characteristics of the coma dust particles.
</p> <p><strong>Results & Conclusions</strong></p> <p>We find that polarisation of 2I/Borisov is higher than is usually measured for Solar System comets.
This distinguishes the interstellar comet from all dynamically evolved comets in our Solar System.
This evidence of 2I/Borisov being more pristine than the observed Solar System comets is corroborated by the fact that the comet with the closest polarimetric properties is C/1995 O1 (Hale–Bopp), which is believed to have approached the Sun only once before its apparition in 1997.
Furthermore, and unlike both Hale–Bopp and many other comets, interstellar comet 2I/Borisov shows a polarimetrically homogeneous coma, unchanging with cometocentric distance, again suggesting it is even more pristine than the observed comets from our own Solar System.
It is thus likely that it has never passed very close to its native star.
</p>.

Related Results

HCREM, a rendezvous mission to comet Halley
HCREM, a rendezvous mission to comet Halley
- IntroductionWe propose a Halley Comet Rendezvous Mission (HCREM) feasible with currently available propulsion technology with a target launch date around 2040. The mission concep...
Comet Dust Tail Analysis using the Finson-Probstein Model
Comet Dust Tail Analysis using the Finson-Probstein Model
The fine-structure detail of several comet dust tails is analysed from amateur and professional comet images using the Finson-Probstein mdoel. Given the date and time of the image ...
Ion velocity distribution functions at a low activity comet
Ion velocity distribution functions at a low activity comet
We study the transition period of induced comet magnetospheres between the simple deflection of the solar wind due to mass loading and a fully developed bow shock. We present exper...
The Moon as an Asteroid: Unlocking Surface Secrets with Atlas Polarimetry
The Moon as an Asteroid: Unlocking Surface Secrets with Atlas Polarimetry
IntroductionThe polarimetric properties of airless Solar System bodies provide invaluable insights into their surface characteristics. While extensively applied to asteroids, often...
Comet C/1908 R1 (Morehouse) as a C/2016 R2 (PanSTARRS)-like comet
Comet C/1908 R1 (Morehouse) as a C/2016 R2 (PanSTARRS)-like comet
IntroductionComets are pristine relics of the early Solar System, formed from the agglomeration of icy grains and dust particles, offering insights into the evolution of the protos...
FeI and NiI in comets
FeI and NiI in comets
Metals have been found in cometary dust by in-situ experiments onboard the Giotto and Rosetta spacecrafts[4,10] as well as in dust particles collected by the Stardust spacecraft[11...
Boulder Mobility on Comets: Insights from Rosetta Observations and Numerical Modelling
Boulder Mobility on Comets: Insights from Rosetta Observations and Numerical Modelling
Boulder displacement on comets, including the migration of rocks up to tens of meters and relocation of decimeter- to meter-scale debris, are critical processes in reshaping the nu...
Polarimetric differential SAR Interferometry with ground-based sensors
Polarimetric differential SAR Interferometry with ground-based sensors
Las técnicas de Interferometría Diferencial se basan en la combinación de varias imágenes SAR con distinta separación temporal y permiten la recuperación de las componentes lineale...

Back to Top