TV observations of the 2018 Draconid meteor shower from Iceland

Abstract Several researchers predicted an outburst of the October Draconids in 2018, with the peak expected between 23:43 UT on October 8 and 00:14 UT on October 9. We observed the event from Husafell, Iceland, where conditions were favorable during the predicted peak time. As a result, we detected the appearance of a more active shower than expected. Three peaks were identified in the time variation of the meteor activity. The main peak occurred at 23:43 UT on October 8, with the estimated hourly rate (HR) reaching 54. This corresponds to a meteor flux of $9.9 \times 10^{-3}\, \mathrm{km^{-2}\, h^{-1}}$ for meteors brighter than +3.5 mag. Two additional sub-peaks were observed at 00:28 and 01:08 UT on October 9. The presence of three distinct peaks suggests a complex structure within the dust trail system. In addition to the main CCD observations, we also employed a complementary observation using a mirrorless digital camera with a high-sensitivity CMOS sensor. The resulting flux values agreed well with those from the CCD system, suggesting that such mirrorless setups may now offer a practical alternative for observing faint meteors.

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Publication Details

Journal
Publications of the Astronomical Society of Japan
Published
2025-11-11
DOI
https://doi.org/10.1093/pasj/psaf112
Primary Topic
Astro and Planetary Science
Type
article
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article

TV observations of the 2018 Draconid meteor shower from Iceland

Mikiya Sato, Chie Tsuchiya, J. Watanabe
Publications of the Astronomical Society of Japan
Astro and Planetary Science
article

TV observations of the 2018 Draconid meteor shower from Iceland

Mikiya Sato, Chie Tsuchiya, J. Watanabe
article en

Abstract

Abstract Several researchers predicted an outburst of the October Draconids in 2018, with the peak expected between 23:43 UT on October 8 and 00:14 UT on October 9. We observed the event from Husafell, Iceland, where conditions were favorable during the predicted peak time. As a result, we detected the appearance of a more active shower than expected. Three peaks were identified in the time variation of the meteor activity. The main peak occurred at 23:43 UT on October 8, with the estimated hourly rate (HR) reaching 54. This corresponds to a meteor flux of $9.9 \times 10^{-3}\, \mathrm{km^{-2}\, h^{-1}}$ for meteors brighter than +3.5 mag. Two additional sub-peaks were observed at 00:28 and 01:08 UT on October 9. The presence of three distinct peaks suggests a complex structure within the dust trail system. In addition to the main CCD observations, we also employed a complementary observation using a mirrorless digital camera with a high-sensitivity CMOS sensor. The resulting flux values agreed well with those from the CCD system, suggesting that such mirrorless setups may now offer a practical alternative for observing faint meteors.

Publications of the Astronomical Society of JapanVol. 78(1)
National Astronomical Observatory of Japan (JP), The University of Tokyo (JP)
Openalex Percentile: Top 77%
Astro and Planetary Science
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