The comet 144P/Kushida

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From Ashburn , 144P/Kushida will become visible around 17:57 (EST), 22° above your south-western horizon, as dusk fades to darkness. It will then sink towards the horizon, setting 3 hours and 37 minutes after the Sun at 20:26.

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Name 144P/Kushida
Object Type Comet
Current Position
Magnitude:23.15 (V) [2]
Absolute mag (H):5.50 [2]
Slope parameter (n):7.48 [2]
Right ascension:19h50m [1]
Declination:-17°53' [1]
Distance:6.03 AU
50.18 lightmin [1]
Orbital Elements [1]
Semi-major axis:3.82 AU
Longitude ascending node:243.15°
Argument of perihelion:216.32°
Epoch of elements:30 November 2021
Mean Anomaly at epoch:256.25°
Derived quantities
Perihelion:1.39 AU
Aphelion:6.25 AU
Orbital period:7.47 years
Visibility from Ashburn

All times shown in Ashburn local time.

13 Dec 2023  –  144P/Kushida at perigee
09 Jan 2024  –  144P/Kushida reaches its brightest
26 Jan 2024  –  144P/Kushida at perihelion
Additional sources

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 For most comets, we do not publish any magnitude estimates at all.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.






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