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11P/Tempel–Swift–LINEAR

Periodic comet


Periodic comet

FieldValue
name11P/Tempel–Swift–LINEAR
image11P 2021-01-04 NEOWISE image 3-color.png
captionInfrared image of Comet T–S–L taken by NEOWISE on 4 January 2021.
discovery_ref
discoverer
discovery_date
mpc_name
designations
orbit_ref
epoch17 October 2024 (JD 2460600.5)
observation_arc154.75 years
obs1,337
perihelion1.388 AU
aphelion5.18 AU
semimajor3.284 AU
eccentricity0.57756
period5.95 years
inclination14.435°
asc_node238.87°
arg_peri168.04°
mean235.14°
tjup2.839
Earth_moid0.403 AU
Jupiter_moid0.326 AU
physical_ref
mean_radius0.6 km
M115.2
M218.6
last_p26 November 2020
next_p9 November 2026

11P/Tempel–Swift–LINEAR is a periodic comet with a 5.95-year orbit around the Sun.

Observational history

Discovery

In 1869, the comet's perihelion was around 1.063 AU from the Sun. Ernst Wilhelm Leberecht Tempel originally discovered the comet on 27 November 1869, from his observatory at Marseille. It was later observed by Lewis Swift from the Warner Observatory on 11 October 1880, and he realised that it is the same comet as Tempel's.

Loss and recovery

After 1908, the comet became an unobservable lost comet due to a series of four close flybys of Jupiter between 1911 and 1946 perturbing its orbit significantly enough that made subsequent apparitions of the comet unfavorable for observations in decades. Nevertheless, Brian G. Marsden computed the resulting orbit based on the observations between 1891 and 1908, and predicted a favorable return in 1963, however the comet remained unobserved. Despite this, additional predictions of the comet's favorable returns were later attempted by Marsden and Zdenek Sekanina in 1971, and Shuichi Nakano in 1995.

On 7 December 2001, an object designated as P/2001 X3 was found by the Lincoln Near-Earth Asteroid Research (LINEAR) program. Analysis of images taken between 10 September and 17 October 2001 later confirmed that P/2001 X3 was the recovery of the previously lost comet Tempel–Swift.

Recent observations

The comet was not observed during the 2008 unfavorable apparition because the perihelion passage occurred when the comet was on the far side of the Sun. The comet was observed during the 2014 and 2020 apparitions. The comet will next come to perihelion on 9 November 2026, then two days later on the 11th, make a closest approach to Earth of 0.4012 AU.

Notes

References

| access-date= 2014-10-28 }}

| doi-access= free }}

| access-date= 2014-10-28 }}

| access-date= 2023-07-12 }}

|access-date=2012-02-19}}

|archive-url=https://web.archive.org/web/20230211111102/https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%2790000219%27&START_TIME=%272026-Nov-09%2018:00%27&STOP_TIME=%272026-Nov-10%2006:00%27&STEP_SIZE=%2710%20minutes%27&QUANTITIES=%2719%27 |archive-date=2023-02-11 |url-status=live

|archive-url=https://web.archive.org/web/20110520032222/http://jcometobs.web.fc2.com/pcmtn/0011p.htm |archive-date=2011-05-20 |url-status=live |access-date=2023-07-27}}

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This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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