 Comet's trajectory through the Solar System, with 30-day motion markers | |
| Discovery[1] | |
|---|---|
| Discovered by | Pan-STARRS |
| Discovery site | Haleakala Observatory |
| Discovery date | 17 March 2018 |
| Designations | |
| C/2018 F4 | |
| hyperbolic comet[2] | |
| Orbital characteristics[2] | |
| Epoch 20 September 2019 (JD 2458746.5) | |
| Observation arc | 1330 days(3.64 years) |
| Perihelion | 3.43997AU |
| Eccentricity | 1.00152 |
| Inclination | 79.0989° |
| Jupiter MOID | 0.596273 AU (89.2012 million km) |
| Physical characteristics[3] | |
| Dimensions | ~0.1–10 km (0.062–6.214 mi) |
C/2018 F4 (PanSTARRS) is ahyperbolic comet (previously classified asA/2018 F4, ahyperbolic asteroid).[2] It was discovered on 17 March 2018 when it was beyond the orbit ofJupiter, 6.4 AU (960 million km) from theSun.[1] It was quite far from the Sun and turned out to simply be an asteroidal object that was discovered beforecometary activity was noticeable. Asperihelion (closest approach to the Sun) is inside the orbit of Jupiter, this object should become more active. In April 2018 it was determined to be a hyperbolic comet.[4] Given that the incoming velocity was similar to that of anOort cloud object, we can very confidently say that it is not of interstellar origin.[5][6] C/2018 F4 fragmented around August 2020.[3][7][8]
It would be no problem to fit aparabolic orbit to the C/2018 F4 data,[2][a] as used to be done for most short arc comets. Theorbital eccentricity is decently constrained at1.0038±0.0072,[a] so it could even be aclosed orbit with an eccentricity below 1.[2] The velocity of the object currently has an uncertainty of ±0.2 km/s. With a common Oort cloud velocity of roughly 3 km/s (6,700 mph) when inbound 200 AU from the Sun, there is no reason to think 2018 F4 is of interstellar origin.[5]
It will come to perihelion around 3 December 2019 when it will be 3.4 AU from the Sun.[2]
Further observations will be necessary to determine if the orbit is hyperbolic. As a comet this object became known as C/2018 F4 (PANSTARRS).
The somewhat shortobservation arc of 35 days suggests that before entering the planetary region of the Solar System (epoch 1950), the comet had an orbital periodon the order of a hundred thousand years. The heliocentric eccentricity became greater than 1 in November 2016 when the comet was 9.6 AU (1.44 billion km) from the Sun.
| Object | Year | Velocity km/s | # of observations andobs arc |
|---|---|---|---|
| 90377 Sedna | 1746 | 1.99±0.00 | 196 in 9240 days |
| C/1980 E1 (Bowell) | 1765 | 2.95±0.00 | 179 in 2514 days |
| C/1997 P2 (Spacewatch) | 1779 | 2.96±0.01 | 94 in 49 days |
| C/2010 X1 (Elenin) | 1798 | 2.96±0.00 | 2,222 in 235 days |
| C/2012 S1 (ISON) | 1801 | 2.99±0.00 | 6,514 in 784 days |
| C/2008 J4 (McNaught) | 1855 | 4.88±5.44 | 22 in 15 days |
| C/2018 F4 | 1792 | 2.74±0.03 | 402 in 967 days |
| C/1999 U2 (SOHO) | 1947 | 17±447 | 41 in 1 day |
| 1I/2017 U1 (ʻOumuamua) | 1982 | 26.49±0.03 | 121 in 34 days |
At 200 AU from the Sun, the escape velocity from the Sun is 2.98 km/s. In the above table, the only outlier isʻOumuamua with a confident 34-day observation arc. Comet C/2008 J4 (McNaught) has a short observation arc with large uncertainties. Comet C/1999 U2 (SOHO) has a meaningless 1-day observation arc. Comet C/2018 F4 has a common Oort cloud velocity when 200 AU from the Sun.[5]
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