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 1 June, at a distance of 0.89 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 3° above the horizon at dawn.

The events that comprise the 1985 apparition of 73P/Schwassmann-Wachmann are as follows:

Date Event
01 May 1985Comet 73P/Schwassmann-Wachmann passes perigee
04 May 1985Comet 73P/Schwassmann-Wachmann reaches peak brightness
01 Jun 1985Comet 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
11 May 1985PegasusVisible from 03:38 until 04:08
Highest at 04:08, 26° above E horizon
13 May 1985PegasusNot observable
15 May 1985PiscesNot observable
17 May 1985PiscesNot observable
19 May 1985PiscesNot observable
21 May 1985PiscesNot observable
23 May 1985CetusNot observable
25 May 1985CetusNot observable
27 May 1985CetusNot observable
29 May 1985CetusNot observable
31 May 1985CetusNot observable
02 Jun 1985CetusNot observable
04 Jun 1985CetusNot observable
06 Jun 1985CetusNot observable
08 Jun 1985CetusNot observable
10 Jun 1985CetusNot observable
12 Jun 1985CetusNot observable
14 Jun 1985CetusNot observable
16 Jun 1985CetusNot observable
18 Jun 1985CetusNot observable
20 Jun 1985CetusNot 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 01h04m30s 4°20'S Cetus 7.5

The coordinates are given in J2000.0.

The sky on 15 Jan 2025

The sky on 15 January 2025
Sunrise
07:08
Sunset
16:36
Twilight ends
18:16
Twilight begins
05:29


Waning Gibbous

95%

16 days old

Planets
Rise Culm. Set
Mercury 06:19 10:48 15:16
Venus 09:20 14:58 20:35
Moon 17:24 01:02 08:28
Mars 16:11 23:56 07:41
Jupiter 13:13 20:41 04:10
Saturn 09:36 15:11 20:47
All times shown in EST.

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 14 Jan 2025.

Image credit

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

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