Comet C/2011 M1 (LINEAR) passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet C/2011 M1 (LINEAR) will make its closest approach to the Sun on 7 September, at a distance of 0.88 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 11° above the horizon at dawn.

The events that comprise the 2011 apparition of C/2011 M1 (LINEAR) are as follows:

Date Event
07 Sep 2011Comet C/2011 M1 (LINEAR) passes perihelion

The table below lists the times when C/2011 M1 (LINEAR) will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
17 Aug 2011Ursa MajorVisible from 20:56 until 04:37
Highest at 04:37, 22° above NE horizon
19 Aug 2011Ursa MajorNot observable
21 Aug 2011Ursa MajorNot observable
23 Aug 2011Ursa MajorNot observable
25 Aug 2011Ursa MajorNot observable
27 Aug 2011Ursa MajorNot observable
29 Aug 2011Ursa MajorNot observable
31 Aug 2011Ursa MajorNot observable
02 Sep 2011Ursa MajorNot observable
04 Sep 2011Ursa MajorNot observable
06 Sep 2011Leo MinorNot observable
08 Sep 2011Leo MinorNot observable
10 Sep 2011Leo MinorNot observable
12 Sep 2011Ursa MajorNot observable
14 Sep 2011Leo MinorNot observable
16 Sep 2011Leo MinorNot observable
18 Sep 2011Leo MinorNot observable
20 Sep 2011Leo MinorNot observable
22 Sep 2011LeoNot observable
24 Sep 2011LeoNot observable
26 Sep 2011LeoNot observable

A more detailed table of C/2011 M1 (LINEAR)'s position on each night is available here. A diagram of the orbit of C/2011 M1 (LINEAR) is available here.

Finder chart

The chart below shows the path of C/2011 M1 (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/2011 M1 (LINEAR) is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2011 M1 (LINEAR) 10h47m30s 37°33'N 9.6

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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