Comet 73P/Schwassmann-Wachmann passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet 73P/Schwassmann-Wachmann will make its closest approach to the Sun on 26 July, at a distance of 0.97 AU.

From Cambridge on the day of perihelion it will not be observable – it will reach its highest point in the sky during daytime and will be no higher than 8° above the horizon at dusk.

The events that comprise the 1984 apparition of 73P/Schwassmann-Wachmann are as follows:

Date Event
26 Jul 1984Comet 73P/Schwassmann-Wachmann passes perihelion

The table below lists the times when 73P/Schwassmann-Wachmann will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
05 Jul 1984LeoNot observable
07 Jul 1984VirgoNot observable
09 Jul 1984VirgoNot observable
11 Jul 1984VirgoNot observable
13 Jul 1984VirgoNot observable
15 Jul 1984VirgoNot observable
17 Jul 1984VirgoNot observable
19 Jul 1984VirgoNot observable
21 Jul 1984VirgoNot observable
23 Jul 1984VirgoNot observable
25 Jul 1984VirgoNot observable
27 Jul 1984VirgoNot observable
29 Jul 1984CorvusNot observable
31 Jul 1984CorvusNot observable
02 Aug 1984VirgoNot observable
04 Aug 1984VirgoNot observable
06 Aug 1984VirgoNot observable
08 Aug 1984VirgoNot observable
10 Aug 1984HydraNot observable
12 Aug 1984HydraNot observable
14 Aug 1984HydraNot observable

A more detailed table of 73P/Schwassmann-Wachmann's position on each night is available here. A diagram of the orbit of 73P/Schwassmann-Wachmann is available here.

Finder chart

The chart below shows the path of 73P/Schwassmann-Wachmann 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 73P/Schwassmann-Wachmann is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet 73P/Schwassmann-Wachmann 12h34m30s 10°11'S Virgo 9.6

The coordinates are given in J2000.0.

The sky on 14 Mar 2025

The sky on 14 March 2025
Sunrise
06:55
Sunset
18:49
Twilight ends
20:23
Twilight begins
05:21


Waning Gibbous

99%

14 days old

Planets
Rise Culm. Set
Mercury 07:15 13:42 20:10
Venus 06:44 13:27 20:09
Moon 18:25 00:49 07:01
Mars 12:49 20:35 04:21
Jupiter 10:30 18:00 01:31
Saturn 07:02 12:47 18:32
All times shown in EDT.

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 23 Feb 2025.

Image credit

© Andy Roberts 1997. Pictured comet is C/1995 O1 Hale-Bopp.

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