15P/Finlay

Description

When the first orbit calculations were made in 1886, there was a similarity between this orbit and that of Francesco de Vico's lost periodic comet of 1844 (54P/de Vico-Swift-NEAT). Lewis Boss (Dudley Observatory, Schenectady, United States) noted large discrepancies between the orbits and after further observations concluded that de Vico's comet could not be the same as Finlay's.

During the 1906 apparition the comet brightened to magnitude 6. In 1910 a close pass with Jupiter increased the orbital period, in 1919 the path was off predictions and a new comet discovered by Sasaki (Kyoto Observatory, Japan) on October 25, 1919, was discovered to be Finlay's.

The magnitude of the comet declined after 1926, and it was not until 1953 that it has been observed on every return.

2014–2015

During the 2014 perihelion passage the comet outburst on 16 December 2014 from magnitude 11 to magnitude 9 becoming bright enough to be seen in common binoculars with a 50 mm objective lens. On December 23, 2014, 15P and Mars were only 1/6 of a degree apart in the sky after sunset. But by December 23, 2014, the comet had dimmed considerably since the outburst. On 16 January 2015, the comet outburst to magnitude 8.

2060

15P/Finlay currently has an Earth-MOID of 0.009 AU.

Arids meteor shower

Debris ejected during the 1995 perihelion passage generated a meteor shower on 29–30 September 2021 radiating from the southern constellation of Ara. More outbursts are expected on 7 October 2021 from the 2008 and 2014 streams.

References

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|author-link=Syuichi Nakano |access-date=2012-02-18}}

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|access-date=2014-12-20|date=2014-12-18}}

|archive-url=https://web.archive.org/web/20170220010657/http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=15P;cad=1 |archive-date=2017-02-20 |url-status=live |access-date=2022-06-16}}

|archive-url=https://archive.today/20150119001956/https://groups.yahoo.com/neo/groups/comets-ml/conversations/messages/24324 |url-status=dead |archive-date=January 19, 2015 |access-date=2015-01-17}}

|archive-url=https://web.archive.org/web/20220616142743/https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%2790000257%27&START_TIME=%272060-Oct-22+17%3A00%27&STOP_TIME=%272060-Oct-22+18%3A00%27&STEP_SIZE=%2710+minutes%27&QUANTITIES=%2720%2C39%27 |archive-date=2022-06-16 |url-status=live

|access-date=2020-07-27}}

|access-date=2021-10-01}}

References

1. (2004). "Comets II". University of Arizona Press.
2. The comet will come to perihelion six more times and then on October 22, 2060, the comet will pass roughly {{convert. 0.0334. AU. e6km e6mi