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7P/Pons–Winnecke

Periodic comet

7P/Pons–Winnecke

Periodic comet

FieldValue
name7P/Pons–Winnecke
image7P 2021-06-08 image ZTF-sso-341-zg-fov-7.0arcmin.png
captionComet Pons–Winnecke as seen in 2021 by ZTF
discovererJean Louis Pons
Friedrich Winnecke
discovery_siteMarseille, France
Bonn, Germany
discovery_date12 June 1819
9 March 1858
mpc_name
designations{{unbulleted1819 III, 1858 II, 1869 I1875 I, 1886 VI,
orbit_ref
epoch25 February 2023 (JD 2460000.5)
observation_arc130.22 years
obs1,797
perihelion1.233 AU
aphelion5.587 AU
semimajor3.410 AU
eccentricity0.63853
period6.296 years
inclination22.373°
asc_node93.327°
arg_peri172.54°
mean100.03°
tjup2.677
Earth_moid0.226 AU
Jupiter_moid0.273 AU
physical_ref
dimensions5.2 km
albedo0.04 (assumed)
rotation6.8–9.5 hours
spectral_type(V–R)
(R–I)
M116.0
last_p27 May 2021
next_p25 August 2027

Friedrich Winnecke Bonn, Germany 9 March 1858 1892 IV|1898 II, 1909 II, 1915 III|1921 III, 1927 VII, 1933 II|1939 V, 1945 IV, 1951 VI|1964 I, 1970 VIII|1976 XIV, 1983 IV|1989 VIII}} (R–I)

7P/Pons–Winnecke (also known as Comet Pons–Winnecke) is a periodic Jupiter-family comet with a six-year orbit around the Sun.

Observational history

Jean Louis Pons (Marseille) originally discovered the comet on 12 June 1819, it was later rediscovered by Friedrich Winnecke (Bonn) on 9 March 1858. It is the parent body of the June Bootids of late June.

PS1921}}

Early calculations for the 1921 apparition suggested that the orbit of the comet might collide with Earth in June, but observations on 10 April ruled out an impact. It made a very close approach to Earth in June 1927. The outward migration of perihelion created impressive meteor showers in 1916, 1921 and 1927.

Orbit

7P currently has an orbital period of 6.3 years. It currently has a perihelion of 1.2 AU (outside the orbit of Earth) and an aphelion of 5.6 AU (past the orbit of Jupiter). It passed within 0.04 AU of Earth in June 1927, and 0.1 AU in 1939; but it will not come as close in the 21st century. A close approach to Jupiter in July 2037 will drop perihelion to 0.982 AU, and by 2062 perihelion will be further reduced to 0.85 AU.

2062

Date & time of
closest approachEarth distance
(AU)Sun distance
(AU)Velocity
wrt Earth
(km/s)Velocity
wrt Sun
(km/s)Uncertainty
region
([3-sigma](3-sigma))Reference
2062-Jun-12 18:25 ± 10 min0.1676 AU0.8499 AU16.342.5± 312 km[Horizons](https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27DES%3D7P%3BCAP%27&START_TIME=%272062-Jun-12%2018:25%27&STOP_TIME=%272062-Jun-13%27&STEP_SIZE=%271%20day%27&QUANTITIES=%2719,20,22,39%27)

The next perihelion passage is 25 August 2027 when the comet will have a solar elongation of 63 degrees. The last perihelion passage was 27 May 2021 when the comet had a solar elongation of 107 degrees at approximately apparent magnitude 11. It passed 0.44 AU from Earth on 12 June 2021. Before that it came to perihelion on 30 January 2015 with a solar elongation of 24 degrees.

Physical characteristics

EpochPerihelion
(AU)
18190.77
18750.83
18860.89
18980.92
19090.97
19211.04
19331.10
19891.26
20271.13
20390.982
20620.847

The comet nucleus is estimated to be 5.2 km in diameter. Photometric measurements from the European Southern Observatory (ESO) reveals that the comet exhibited brightness variations, which imply that its rotation period is roughly between 6.8–9.5 hours. Dust production rate was measured to be less than 150 kg/s during its 2021 apparition.

Proposed exploration

''Mariner 5''

The Jet Propulsion Laboratory proposed a flyby of the comet with a flight spare of Mariner 4 with the closest approach taking place in 1969 at a distance of 5000 km. However, the intrinsically faint comet's ephemeris was poorly defined at the time, making it difficult to track its position optically from the ground. The probe was instead used for a 1967 Venus flyby as Mariner 5.

In 2019, 7P/Pons–Winnecke was listed as one of 10 backup targets of the European Space Agency's Comet Interceptor mission. Scheduled for launch on 2029, the spacecraft may conduct a flyby of 7P on 28 September 2033 if selected.

References

| access-date= 2 May 2025 }}

| access-date= 5 March 2019 }}

| access-date= 5 March 2019 }}

| display-authors= 4

| display-authors= etal | doi-access= free }}

| doi-access= free }}

https://books.google.com/books?id=Fi1mCYJWBwAC&pg=PA57

|access-date=2014-10-29}}

|archive-url=https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%2790000167%27&START_TIME=%272027-Aug-25%27&STOP_TIME=%272027-Aug-27%27&STEP_SIZE=%2720%20minutes%27&QUANTITIES=%2719%27 |archive-date=2022-06-15 |url-status=live

|archive-url=https://web.archive.org/web/20110520033132/http://jcometobs.web.fc2.com/pcmtn/0007p.htm |archive-date=2011-05-20 |url-status=live |access-date=2023-07-27}}

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