Comet C/2011 L4 (PANSTARRS) passes perigee

Dominic Ford, Editor
From the Comets feed


Comet C/2011 L4 (PANSTARRS) will make its closest approach to the Earth on 4 March, at a distance of of 1.09 AU.

From Cambridge on the day of perigee it will not be observable – it will reach its highest point in the sky during daytime and will be 5° below the horizon at dusk.

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

Date Event
04 Mar 2013Comet C/2011 L4 (PANSTARRS) passes perigee
08 Mar 2013Comet C/2011 L4 (PANSTARRS) passes perihelion

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

Date Constellation Comet visibility
11 Feb 2013MicroscopiumNot observable
13 Feb 2013MicroscopiumNot observable
15 Feb 2013MicroscopiumNot observable
17 Feb 2013GrusNot observable
19 Feb 2013GrusNot observable
21 Feb 2013GrusNot observable
23 Feb 2013Piscis AustrinusNot observable
25 Feb 2013Piscis AustrinusNot observable
27 Feb 2013SculptorNot observable
01 Mar 2013SculptorNot observable
03 Mar 2013AquariusNot observable
05 Mar 2013CetusNot observable
07 Mar 2013CetusNot observable
09 Mar 2013PiscesNot observable
11 Mar 2013PiscesVisible from 19:03 until 19:06
Highest at 19:03, 8° above W horizon
13 Mar 2013PiscesVisible from 19:08 until 19:17
Highest at 19:08, 10° above W horizon
15 Mar 2013PiscesVisible from 19:15 until 19:24
Highest at 19:15, 11° above W horizon
17 Mar 2013PiscesVisible from 19:22 until 19:28
Highest at 19:22, 11° above W horizon
19 Mar 2013PiscesNot observable
21 Mar 2013AndromedaNot observable
23 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 perigee will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2011 L4 (PANSTARRS) 23h54m40s 17°09'S Aquarius 0.9

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

98%

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.

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 23 Feb 2025.

Image credit

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

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