Comet C/2011 W3 (Lovejoy) passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet C/2011 W3 (Lovejoy) will make its closest approach to the Sun on 15 December, at a distance of 0.06 AU.

From South El Monte on the day of perihelion it will not be readily observable since it will be very close to the Sun, at a separation of only 3° from it.

The events that comprise the 2011–2012 apparition of C/2011 W3 (Lovejoy) are as follows:

Date Event
15 Dec 2011Comet C/2011 W3 (Lovejoy) passes perihelion

The table below lists the times when C/2011 W3 (Lovejoy) will be visible from South El Monte day-by-day through its apparition:

Date Constellation Comet visibility
24 Nov 2011CentaurusNot observable
26 Nov 2011CentaurusNot observable
28 Nov 2011CentaurusNot observable
30 Nov 2011CentaurusNot observable
02 Dec 2011LupusNot observable
04 Dec 2011LupusNot observable
06 Dec 2011NormaNot observable
08 Dec 2011ScorpiusNot observable
10 Dec 2011ScorpiusNot observable
12 Dec 2011ScorpiusNot observable
14 Dec 2011OphiuchusNot observable
16 Dec 2011OphiuchusNot observable
18 Dec 2011OphiuchusNot observable
20 Dec 2011ScorpiusNot observable
22 Dec 2011ScorpiusNot observable
24 Dec 2011ScorpiusNot observable
26 Dec 2011AraNot observable
28 Dec 2011AraNot observable
30 Dec 2011AraNot observable
01 Jan 2012Triangulum AustraleNot observable
03 Jan 2012ApusNot observable

A more detailed table of C/2011 W3 (Lovejoy)'s position on each night is available here. A diagram of the orbit of C/2011 W3 (Lovejoy) is available here.

Finder chart

The chart below shows the path of C/2011 W3 (Lovejoy) 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 W3 (Lovejoy) is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2011 W3 (Lovejoy) 17h16m10s 23°52'S Ophiuchus -9.8

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

87%

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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