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

Comet 88P/Howell passes perihelion

Dominic Ford, Editor
From the Comets feed

Objects: 88P/Howell
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Comet 88P/Howell will make its closest approach to the Sun on 12 October, 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 10° above the horizon at dusk.

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The events that comprise the 2009 apparition of 88P/Howell are as follows:

Date Event
12 Oct 2009Comet 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
21 Sep 2009LibraNot observable
23 Sep 2009LibraNot observable
25 Sep 2009ScorpiusNot observable
27 Sep 2009ScorpiusNot observable
29 Sep 2009ScorpiusNot observable
01 Oct 2009ScorpiusNot observable
03 Oct 2009ScorpiusNot observable
05 Oct 2009OphiuchusNot observable
07 Oct 2009ScorpiusNot observable
09 Oct 2009ScorpiusNot observable
11 Oct 2009ScorpiusNot observable
13 Oct 2009OphiuchusNot observable
15 Oct 2009OphiuchusNot observable
17 Oct 2009OphiuchusNot observable
19 Oct 2009OphiuchusNot observable
21 Oct 2009OphiuchusNot observable
23 Oct 2009OphiuchusNot observable
25 Oct 2009OphiuchusNot observable
27 Oct 2009SagittariusNot observable
29 Oct 2009SagittariusNot observable
31 Oct 2009SagittariusNot 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 16h53m50s 25°36'S Ophiuchus 8.9

The coordinates are given in J2000.0.

The sky on 27 Apr 2024

The sky on 27 April 2024
Sunrise
05:42
Sunset
19:39
Twilight ends
21:27
Twilight begins
03:54

19-day old moon
Waning Gibbous

80%

19 days old

Planets
Rise Culm. Set
Mercury 05:01 11:21 17:40
Venus 05:25 12:03 18:41
Moon 22:55 03:15 07:31
Mars 04:17 10:12 16:07
Jupiter 06:31 13:42 20:54
Saturn 03:54 09:31 15:08
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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