C/2020 V2 (Comet)
From Fairfield , C/2020 V2 will become visible around 21:38 (EDT), 54° above your north-western horizon, as dusk fades to darkness. It will then sink towards the horizon, becoming tricky to observe after 02:16 when it dips 21° above your north-western horizon.
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Name
C/2020 V2
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Object type
Comet
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| Constellation: | Ursa Major |
| Magnitude: | 13.57 (V) [2] |
| Absolute mag (H): | 4.00 [2] |
| Slope parameter (n): | 3.96 [2] |
| Right ascension: | 09h58m [1] |
| Declination: | +58°39' [1] |
| Distance: | 4.56 AU 37.91 lightmin [1] |
| Semi-major axis: | -2046.04 AU |
| Eccentricity: | 1.001089 |
| Inclination: | 131.61° |
| Longitude ascending node: | 212.37° |
| Argument of perihelion: | 162.41° |
| Epoch of elements: | 28 May 2022 |
| Mean Anomaly at epoch: | 360.00° |
| Perihelion: | 2.23 AU |
All times shown in Fairfield local time.
| 08 May 2023 | – C/2020 V2 (ZTF) at perihelion |
The position of this comet was calculated from orbital elements published by the Minor Planet Center (MPC).
We estimate the brightnesses of comets from magnitude parameters published by the BAA Comet Section, where these are available. These are computed from the observations they receive from amateur astronomers.
Comets are intrinsically highly unpredictable objects, since their brightness depends on the scattering of sunlight from dust particles in the comet's coma and tail. This dust is continually streaming away from the comet's nucleus, and its density at any particular time is governed by the rate of sublimation of the ice in the comet's nucleus, as it is heated by the Sun's rays. It also depends on the amount of dust that is mixed in with that ice. This is very difficult to predict in advance, and can be highly variable even between successive apparitions of the same comet.
In consequence, while the future positions of comets are usually known with a high degree of confidence, their future brightnesses are not. For most comets, we do not publish any magnitude estimates at all. For the few comets where we do make estimates, we generally prefer the BAA's magnitude parameters to those published by the Minor Planet Center, since they are typically updated more often.