Comet 10P/Tempel passes perihelion

Dominic Ford, Editor
From the Comets feed


Objects: 10P/Tempel

Comet 10P/Tempel will make its closest approach to the Sun on 2 June, at a distance of 1.42 AU.

From Fairfield 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 17° above the horizon at dawn.

The events that comprise the 1994 apparition of 10P/Tempel are as follows:

Date Event
02 Jun 1994Comet 10P/Tempel passes perihelion

The table below lists the times when 10P/Tempel will be visible from Fairfield day-by-day through its apparition:

Date Constellation Comet visibility
12 May 1994AquariusNot observable
14 May 1994AquariusNot observable
16 May 1994AquariusNot observable
18 May 1994AquariusNot observable
20 May 1994AquariusNot observable
22 May 1994AquariusNot observable
24 May 1994AquariusNot observable
26 May 1994AquariusNot observable
28 May 1994AquariusNot observable
30 May 1994AquariusNot observable
01 Jun 1994AquariusNot observable
03 Jun 1994PiscesNot observable
05 Jun 1994PiscesNot observable
07 Jun 1994PiscesNot observable
09 Jun 1994PiscesNot observable
11 Jun 1994PiscesNot observable
13 Jun 1994CetusNot observable
15 Jun 1994CetusNot observable
17 Jun 1994CetusNot observable
19 Jun 1994CetusNot observable
21 Jun 1994CetusVisible from 03:53 until 03:54
Highest at 03:54, 22° above SE horizon

A more detailed table of 10P/Tempel's position on each night is available here. A diagram of the orbit of 10P/Tempel is available here.

Finder chart

The chart below shows the path of 10P/Tempel 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 10P/Tempel is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet 10P/Tempel 23h53m50s 4°29'S Aquarius 9.8

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

36%

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 13 Oct 2024.

Image credit

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

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