Comet C/2002 T7 (LINEAR) passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet C/2002 T7 (LINEAR) will make its closest approach to the Sun on 26 April, at a distance of 0.64 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 4° above the horizon at dawn.

The events that comprise the 2004 apparition of C/2002 T7 (LINEAR) are as follows:

Date Event
26 Apr 2004Comet C/2002 T7 (LINEAR) passes perihelion
21 May 2004Comet C/2002 T7 (LINEAR) passes perigee
21 May 2004Comet C/2002 T7 (LINEAR) reaches peak brightness

The table below lists the times when C/2002 T7 (LINEAR) will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
05 Apr 2004PiscesNot observable
07 Apr 2004PiscesNot observable
09 Apr 2004PiscesNot observable
11 Apr 2004PiscesNot observable
13 Apr 2004PiscesNot observable
15 Apr 2004PiscesNot observable
17 Apr 2004PiscesNot observable
19 Apr 2004PiscesNot observable
21 Apr 2004PiscesNot observable
23 Apr 2004PiscesNot observable
25 Apr 2004PiscesNot observable
27 Apr 2004PiscesNot observable
29 Apr 2004PiscesNot observable
01 May 2004PiscesNot observable
03 May 2004PiscesNot observable
05 May 2004PiscesNot observable
07 May 2004PiscesNot observable
09 May 2004CetusNot observable
11 May 2004CetusNot observable
13 May 2004CetusNot observable
15 May 2004CetusNot observable

A more detailed table of C/2002 T7 (LINEAR)'s position on each night is available here. A diagram of the orbit of C/2002 T7 (LINEAR) is available here.

Finder chart

The chart below shows the path of C/2002 T7 (LINEAR) 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 C/2002 T7 (LINEAR) is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2002 T7 (LINEAR) 23h58m40s 4°08'N Pisces 4.4

The coordinates are given in J2000.0.

The sky on 14 Mar 2025

The sky on 14 March 2025
Sunrise
06:55
Sunset
18:49
Twilight ends
20:23
Twilight begins
05:21


Waning Gibbous

99%

14 days old

Planets
Rise Culm. Set
Mercury 07:15 13:42 20:10
Venus 06:44 13:27 20:09
Moon 18:25 00:49 07:01
Mars 12:49 20:35 04:21
Jupiter 10:30 18:00 01:31
Saturn 07:02 12:47 18:32
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 23 Feb 2025.

Image credit

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

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