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

Comet 73P/Schwassmann-Wachmann passes perihelion

Dominic Ford, Editor
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Comet 73P/Schwassmann-Wachmann will make its closest approach to the Sun on 17 July, at a distance of 0.96 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.

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The events that comprise the 1995 apparition of 73P/Schwassmann-Wachmann are as follows:

Date Event
17 Jul 1995Comet 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
26 Jun 1995LeoVisible from 21:55 until 22:14
Highest at 21:55, 25° above W horizon
28 Jun 1995LeoVisible from 21:54 until 22:06
Highest at 21:54, 24° above W horizon
30 Jun 1995LeoVisible from 21:54 until 21:58
Highest at 21:54, 23° above W horizon
02 Jul 1995LeoNot observable
04 Jul 1995LeoNot observable
06 Jul 1995LeoNot observable
08 Jul 1995VirgoNot observable
10 Jul 1995VirgoNot observable
12 Jul 1995VirgoNot observable
14 Jul 1995VirgoNot observable
16 Jul 1995VirgoNot observable
18 Jul 1995VirgoNot observable
20 Jul 1995VirgoNot observable
22 Jul 1995VirgoNot observable
24 Jul 1995CorvusNot observable
26 Jul 1995CorvusNot observable
28 Jul 1995CorvusNot observable
30 Jul 1995CorvusNot observable
01 Aug 1995CorvusNot observable
03 Aug 1995VirgoNot observable
05 Aug 1995HydraNot 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 12h02m10s 9°05'S Virgo 8.8

The coordinates are given in J2000.0.

The sky on 11 May 2024

The sky on 11 May 2024
Sunrise
05:24
Sunset
19:55
Twilight ends
21:51
Twilight begins
03:28

3-day old moon
Waxing Crescent

20%

3 days old

Planets
Rise Culm. Set
Mercury 04:34 11:02 17:29
Venus 05:13 12:14 19:15
Moon 07:46 16:04 00:19
Mars 03:46 09:56 16:07
Jupiter 05:46 13:01 20:16
Saturn 03:02 08:40 14:19
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 27 Apr 2024.

Image credit

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

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Cambridge

Latitude:
Longitude:
Timezone:

42.38°N
71.11°W
EDT

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