Comet 71P/Clark passes perihelion

Dominic Ford, Editor
From the Comets feed


Objects: 71P/Clark

Comet 71P/Clark will make its closest approach to the Sun on 27 May, at a distance of 1.60 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 19° above the horizon.

The events that comprise the 1989 apparition of 71P/Clark are as follows:

Date Event
27 May 1989Comet 71P/Clark passes perihelion

The table below lists the times when 71P/Clark will be visible from Fairfield day-by-day through its apparition:

Date Constellation Comet visibility
06 May 1989CapricornusNot observable
08 May 1989CapricornusNot observable
10 May 1989CapricornusNot observable
12 May 1989CapricornusNot observable
14 May 1989CapricornusNot observable
16 May 1989CapricornusNot observable
18 May 1989CapricornusNot observable
20 May 1989CapricornusNot observable
22 May 1989CapricornusNot observable
24 May 1989CapricornusNot observable
26 May 1989CapricornusNot observable
28 May 1989CapricornusNot observable
30 May 1989CapricornusNot observable
01 Jun 1989CapricornusNot observable
03 Jun 1989Piscis AustrinusNot observable
05 Jun 1989Piscis AustrinusNot observable
07 Jun 1989Piscis AustrinusNot observable
09 Jun 1989Piscis AustrinusNot observable
11 Jun 1989Piscis AustrinusNot observable
13 Jun 1989Piscis AustrinusNot observable
15 Jun 1989Piscis AustrinusNot observable

A more detailed table of 71P/Clark's position on each night is available here. A diagram of the orbit of 71P/Clark is available here.

Finder chart

The chart below shows the path of 71P/Clark 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 71P/Clark is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet 71P/Clark 20h13m10s 29°46'S Sagittarius 9.0

The coordinates are given in J2000.0.

The sky on 23 Nov 2024

The sky on 23 November 2024
Sunrise
06:48
Sunset
16:27
Twilight ends
18:04
Twilight begins
05:11


Waning Crescent

35%

22 days old

Planets
Rise Culm. Set
Mercury 08:37 13:04 17:30
Venus 10:14 14:41 19:08
Moon 23:20 06:15 12:58
Mars 20:49 04:12 11:35
Jupiter 17:22 00:49 08:16
Saturn 13:05 18:37 00:09
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 19 Oct 2024.

Image credit

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

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