Comet 45P/Honda-Mrkos-Pajdusakova passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet 45P/Honda-Mrkos-Pajdusakova will make its closest approach to the Sun on 31 December, at a distance of 0.56 AU.

From South El Monte on the day of perihelion it will be visible in the morning sky, becoming accessible around 20:46, when it reaches an altitude of 21° above your eastern horizon. It will then reach its highest point in the sky at 01:46, 73° above your southern horizon. It will be lost to dawn twilight around 05:54, 32° above your western horizon.

The events that comprise the 1969–1970 apparition of 45P/Honda-Mrkos-Pajdusakova are as follows:

Date Event

The table below lists the times when 45P/Honda-Mrkos-Pajdusakova will be visible from South El Monte day-by-day through its apparition:

Date Constellation Comet visibility
10 Aug 2027OrionVisible from 04:53 until 05:02
Highest at 05:02, 24° above E horizon
12 Aug 2027GeminiVisible from 05:00 until 05:04
Highest at 05:04, 23° above E horizon
14 Aug 2027GeminiNot observable
16 Aug 2027GeminiNot observable
18 Aug 2027GeminiNot observable
20 Aug 2027GeminiNot observable
22 Aug 2027GeminiNot observable
24 Aug 2027GeminiNot observable
26 Aug 2027CancerNot observable
28 Aug 2027CancerNot observable
30 Aug 2027CancerNot observable
01 Sep 2027CancerNot observable
03 Sep 2027CancerNot observable
05 Sep 2027CancerNot observable
07 Sep 2027CancerNot observable
09 Sep 2027LeoNot observable
11 Sep 2027LeoNot observable
13 Sep 2027LeoNot observable
15 Sep 2027LeoNot observable
17 Sep 2027LeoNot observable
19 Sep 2027LeoNot observable

A more detailed table of 45P/Honda-Mrkos-Pajdusakova's position on each night is available here. A diagram of the orbit of 45P/Honda-Mrkos-Pajdusakova is available here.

Finder chart

The chart below shows the path of 45P/Honda-Mrkos-Pajdusakova 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 45P/Honda-Mrkos-Pajdusakova is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet 45P/Honda-Mrkos-Pajdusakova 08h32m30s 17°33'N Cancer 8.0

The coordinates are given in J2000.0.

The sky on 10 Oct 2025

The sky on 10 October 2025
Sunrise
06:51
Sunset
18:23
Twilight ends
19:47
Twilight begins
05:27


Waning Gibbous

79%

19 days old

Planets
Rise Culm. Set
Mercury 08:22 13:45 19:07
Venus 05:09 11:20 17:31
Moon 20:08 03:33 11:06
Mars 08:52 14:12 19:31
Jupiter 00:09 07:14 14:19
Saturn 17:30 23:23 05:16
All times shown in PDT.

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 29 Sep 2025.

Image credit

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

Share