15P/Finlay

When the first orbit calculations were made in 1886, there was a similarity between this orbit and that of Francesco de Vico's lost comet of 1844.^[a] Lewis Boss noted large discrepancies between the orbits and after further observations concluded that de Vico's comet could not be the same as Finlay's.^[7]

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 25 October 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.

In 2004, Jakub Cerny estimated that the nucleus of 15P/Finlay has an upper limit of about 1.5 km (0.93 mi) using non-gravitational forces to determine it.^[11] However this was uncertain as it assumed a nearly 10% active surface fraction upon perihelion.^[11] Photometric data in 2000 obtained an absolute magnitude of 17.2, which corresponds to a much larger nucleus at 2.42 km (1.50 mi) assuming its geometric albedo is around 0.035.^[5]

Debris ejected during the 1995 perihelion passage generated a meteor shower on 29–30 September 2021 radiating from the southern constellation of Ara.^[12][13] More outbursts are expected on 7 October 2021 from the 2008 and 2014 streams.^[14]

A 2026 study confirmed that this meteor shower was successfully detected at the Mauna Kea Observatory in Hawaii, where the source was attributed to have originated from dust ejected during the 2014 apparition of Finlay.^[15] However the study also noted that the 2008 apparition was exceptionally quiet, making it unlikely to have produced high-velocity dust that could have contributed to the 2021 meteor shower as the 2014 apparition did.^[15]