On the extremely low polarization in Comet C/2023 P1 (Nishimura)

Author:

Zheltobryukhov Maxim1ORCID,Zubko Evgenij2ORCID,Chornaya Ekaterina1ORCID,Kochergin Anton1ORCID,Hines Dean C3,Videen Gorden4

Affiliation:

1. Institute of Applied Astronomy of Russian Academy of Science , 10 Kutuzova Emb., Saint-Petersburg 191187 , Russia

2. Planetary Atmospheres Group, Institute for Basic Science (IBS) , 55 Expo-ro, Yuseong-gu, Daejeon 34126 , South Korea

3. Space Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218 , USA

4. Space Science Institute , 4750 Walnut Street, Boulder Suite 205, CO 80301 , USA

Abstract

ABSTRACT On September 6 and 7 of 2023, we measured the degree of linear polarization of Comet C/2023 P1 (Nishimura) with the R filter. Our observations reveal an extremely low amplitude of positive polarization. Our modelling suggests Mg-rich silicate dust particles are the dominant species in the coma; whereas, an alternative explanation is that such low positive polarization in comets is attributed to the depolarizing effect of their gaseous emission. These two alternative explanations predict dramatically different polarimetric responses at small phase angle that can be discriminated in future polarimetric observations of Comet C/2023 P1 (Nishimura).

Funder

Institute for Basic Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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