1,399 days ago
Dominic Ford, Editor
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Comet C/2021 A2 (NEOWISE) will make its closest approach to the Sun on 22 January, at a distance of 1.41 AU.
From Fairfield on the day of perihelion it will not be readily observable since it will lie so far south that it will never rise more than 11° above the horizon.
The events that comprise the 2020–2021 apparition of C/2021 A2 (NEOWISE) are as follows:
Date | Event |
22 Jan 2021 | Comet C/2021 A2 (NEOWISE) passes perihelion |
The table below lists the times when C/2021 A2 (NEOWISE) will be visible from Fairfield day-by-day through its apparition:
Date | Constellation | Comet visibility |
01 Jan 2021 | Vela | Not observable |
03 Jan 2021 | Vela | Not observable |
05 Jan 2021 | Vela | Not observable |
07 Jan 2021 | Vela | Not observable |
09 Jan 2021 | Vela | Not observable |
11 Jan 2021 | Vela | Not observable |
13 Jan 2021 | Vela | Not observable |
15 Jan 2021 | Vela | Not observable |
17 Jan 2021 | Vela | Not observable |
19 Jan 2021 | Vela | Not observable |
21 Jan 2021 | Vela | Not observable |
23 Jan 2021 | Pyxis | Not observable |
25 Jan 2021 | Pyxis | Not observable |
27 Jan 2021 | Puppis | Visible from 23:15 until 00:03 Highest at 23:39, 22° above S horizon |
29 Jan 2021 | Puppis | Visible from 21:22 until 01:06 Highest at 23:14, 27° above S horizon |
31 Jan 2021 | Puppis | Visible from 20:12 until 01:27 Highest at 22:49, 33° above S horizon |
02 Feb 2021 | Monoceros | Visible from 19:13 until 01:38 Highest at 22:26, 38° above S horizon |
04 Feb 2021 | Monoceros | Visible from 18:22 until 01:43 Highest at 22:02, 44° above S horizon |
06 Feb 2021 | Monoceros | Visible from 18:22 until 01:45 Highest at 21:40, 50° above S horizon |
08 Feb 2021 | Monoceros | Visible from 18:25 until 01:43 Highest at 21:19, 55° above S horizon |
10 Feb 2021 | Monoceros | Visible from 18:27 until 01:41 Highest at 20:59, 60° above S horizon |
A more detailed table of C/2021 A2 (NEOWISE)'s position on each night is available here. A diagram of the orbit of C/2021 A2 (NEOWISE) is available here.
Finder chart
The chart below shows the path of C/2021 A2 (NEOWISE) over the course of its apparition, as calculated from the orbital elements published by the Minor Planet Center (MPC). It is available for download, either on dark background, in PNG, PDF or SVG formats, or on a light background, in PNG, PDF or SVG formats. It was produced using StarCharter.
Comet brightnesses
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.
No estimate for the brightness of comet C/2021 A2 (NEOWISE) is currently available.
The comet's position at perihelion will be:
Object | Right Ascension | Declination | Constellation | Magnitude |
Comet C/2021 A2 (NEOWISE) | 09h03m10s | 37°21'S | Vela | 11.2 |
The coordinates are given in J2000.0.
The sky on 22 Jan 2021
The sky on 22 January 2021 | ||||||||||||||||||||||||||||||||||
71% 9 days old |
All times shown in EST.
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Source
This event was automatically generated on the basis of orbital elements published by the Minor Planet Center (MPC) , and is updated whenever new elements become available. It was last updated on 12 Nov 2024.
Image credit
© Andy Roberts 1997. Pictured comet is C/1995 O1 Hale-Bopp.