Comet 88P/Howell passes perihelion

Dominic Ford, Editor
From the Comets feed


Objects: 88P/Howell

Comet 88P/Howell will make its closest approach to the Sun on 3 April, at a distance of 1.36 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 2015 apparition of 88P/Howell are as follows:

Date Event
03 Apr 2015Comet 88P/Howell passes perihelion

The table below lists the times when 88P/Howell will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
13 Mar 2015CapricornusNot observable
15 Mar 2015CapricornusNot observable
17 Mar 2015CapricornusNot observable
19 Mar 2015CapricornusNot observable
21 Mar 2015CapricornusNot observable
23 Mar 2015CapricornusNot observable
25 Mar 2015CapricornusNot observable
27 Mar 2015CapricornusNot observable
29 Mar 2015CapricornusNot observable
31 Mar 2015CapricornusNot observable
02 Apr 2015CapricornusNot observable
04 Apr 2015CapricornusNot observable
06 Apr 2015AquariusNot observable
08 Apr 2015AquariusNot observable
10 Apr 2015AquariusNot observable
12 Apr 2015AquariusNot observable
14 Apr 2015AquariusNot observable
16 Apr 2015AquariusNot observable
18 Apr 2015AquariusNot observable
20 Apr 2015AquariusNot observable
22 Apr 2015AquariusNot observable

A more detailed table of 88P/Howell's position on each night is available here. A diagram of the orbit of 88P/Howell is available here.

Finder chart

The chart below shows the path of 88P/Howell 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 88P/Howell is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet 88P/Howell 21h54m30s 15°36'S Capricornus 9.1

The coordinates are given in J2000.0.

The sky on 23 Nov 2024

The sky on 23 November 2024
Sunrise
06:43
Sunset
16:15
Twilight ends
17:54
Twilight begins
05:03


Waning Crescent

36%

22 days old

Planets
Rise Culm. Set
Mercury 08:33 12:55 17:17
Venus 10:09 14:32 18:54
Moon 23:09 06:06 12:50
Mars 20:36 04:03 11:30
Jupiter 17:09 00:40 08:11
Saturn 12:58 18:29 23:59
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 13 Oct 2024.

Image credit

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

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