Comet C/2011 L4 (PANSTARRS) passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet C/2011 L4 (PANSTARRS) will make its closest approach to the Sun on 9 March, at a distance of 0.30 AU.

From South El Monte 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 dusk.

The events that comprise the 2013 apparition of C/2011 L4 (PANSTARRS) are as follows:

Date Event
05 Mar 2013Comet C/2011 L4 (PANSTARRS) passes perigee
09 Mar 2013Comet C/2011 L4 (PANSTARRS) passes perihelion

The table below lists the times when C/2011 L4 (PANSTARRS) will be visible from South El Monte day-by-day through its apparition:

Date Constellation Comet visibility
16 Feb 2013GrusNot observable
18 Feb 2013GrusNot observable
20 Feb 2013GrusNot observable
22 Feb 2013GrusNot observable
24 Feb 2013Piscis AustrinusNot observable
26 Feb 2013SculptorNot observable
28 Feb 2013SculptorNot observable
02 Mar 2013AquariusNot observable
04 Mar 2013AquariusNot observable
06 Mar 2013CetusNot observable
08 Mar 2013CetusNot observable
10 Mar 2013PiscesVisible from 19:11 until 19:17
Highest at 19:11, 9° above W horizon
12 Mar 2013PiscesVisible from 19:13 until 19:27
Highest at 19:13, 11° above W horizon
14 Mar 2013PiscesVisible from 19:17 until 19:32
Highest at 19:17, 12° above W horizon
16 Mar 2013PiscesVisible from 19:22 until 19:34
Highest at 19:22, 11° above W horizon
18 Mar 2013PiscesVisible from 19:28 until 19:33
Highest at 19:28, 11° above W horizon
20 Mar 2013PiscesNot observable
22 Mar 2013AndromedaNot observable
24 Mar 2013AndromedaNot observable
26 Mar 2013AndromedaNot observable
28 Mar 2013AndromedaNot observable

A more detailed table of C/2011 L4 (PANSTARRS)'s position on each night is available here. A diagram of the orbit of C/2011 L4 (PANSTARRS) is available here.

Finder chart

The chart below shows the path of C/2011 L4 (PANSTARRS) 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/2011 L4 (PANSTARRS) is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2011 L4 (PANSTARRS) 00h20m20s 4°29'S Pisces 0.7

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.

Warning

Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.

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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