Comet C/2012 F6 (Lemmon) passes perigee

Dominic Ford, Editor
From the Comets feed


Comet C/2012 F6 (Lemmon) will make its closest approach to the Earth on 5 February, at a distance of of 0.97 AU.

From South El Monte on the day of perigee it will not be observable because it will lie so far south that it never rises above the horizon.

The events that comprise the 2013 apparition of C/2012 F6 (Lemmon) are as follows:

Date Event
05 Feb 2013Comet C/2012 F6 (Lemmon) passes perigee
17 Mar 2013Comet C/2012 F6 (Lemmon) reaches peak brightness
24 Mar 2013Comet C/2012 F6 (Lemmon) passes perihelion

The table below lists the times when C/2012 F6 (Lemmon) will be visible from South El Monte day-by-day through its apparition:

Date Constellation Comet visibility
15 Jan 2013CentaurusNot observable
17 Jan 2013CentaurusNot observable
19 Jan 2013CruxNot observable
21 Jan 2013CruxNot observable
23 Jan 2013MuscaNot observable
25 Jan 2013MuscaNot observable
27 Jan 2013MuscaNot observable
29 Jan 2013ChamaeleonNot observable
31 Jan 2013ChamaeleonNot observable
02 Feb 2013ChamaeleonNot observable
04 Feb 2013OctansNot observable
06 Feb 2013OctansNot observable
08 Feb 2013OctansNot observable
10 Feb 2013OctansNot observable
12 Feb 2013OctansNot observable
14 Feb 2013TucanaNot observable
16 Feb 2013TucanaNot observable
18 Feb 2013TucanaNot observable
20 Feb 2013TucanaNot observable
22 Feb 2013TucanaNot observable
24 Feb 2013TucanaNot observable

A more detailed table of C/2012 F6 (Lemmon)'s position on each night is available here. A diagram of the orbit of C/2012 F6 (Lemmon) is available here.

Finder chart

The chart below shows the path of C/2012 F6 (Lemmon) 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/2012 F6 (Lemmon) is currently available.

The comet's position at perigee will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2012 F6 (Lemmon) 17h01m50s 87°21'S Octans 5.8

The coordinates are given in J2000.0.

The sky on 28 Jan 2026

The sky on 28 January 2026
Sunrise
06:49
Sunset
17:17
Twilight ends
18:44
Twilight begins
05:23


Waxing Gibbous

88%

10 days old

Planets
Rise Culm. Set
Mercury 07:16 12:26 17:36
Venus 07:14 12:26 17:38
Moon 12:50 20:27 04:06
Mars 06:40 11:45 16:50
Jupiter 15:24 22:33 05:41
Saturn 09:20 15:15 21:10
All times shown in PST.

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 15 Dec 2025.

Image credit

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

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