Comet C/2015 G2 (MASTER) passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet C/2015 G2 (MASTER) will make its closest approach to the Sun on 25 May, at a distance of 0.77 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 14° below the horizon at dusk.

The events that comprise the 2015 apparition of C/2015 G2 (MASTER) are as follows:

Date Event
14 May 2015Comet C/2015 G2 (MASTER) passes perigee
15 May 2015Comet C/2015 G2 (MASTER) reaches peak brightness
25 May 2015Comet C/2015 G2 (MASTER) passes perihelion

The table below lists the times when C/2015 G2 (MASTER) will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
04 May 2015SculptorNot observable
06 May 2015SculptorNot observable
08 May 2015SculptorNot observable
10 May 2015SculptorNot observable
12 May 2015FornaxNot observable
14 May 2015FornaxNot observable
16 May 2015EridanusNot observable
18 May 2015EridanusNot observable
20 May 2015LepusNot observable
22 May 2015LepusNot observable
24 May 2015Canis MajorNot observable
26 May 2015Canis MajorNot observable
28 May 2015MonocerosNot observable
30 May 2015MonocerosNot observable
01 Jun 2015MonocerosNot observable
03 Jun 2015MonocerosNot observable
05 Jun 2015MonocerosNot observable
07 Jun 2015MonocerosNot observable
09 Jun 2015Canis MinorNot observable
11 Jun 2015Canis MinorNot observable
13 Jun 2015Canis MinorNot observable

A more detailed table of C/2015 G2 (MASTER)'s position on each night is available here. A diagram of the orbit of C/2015 G2 (MASTER) is available here.

Finder chart

The chart below shows the path of C/2015 G2 (MASTER) 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/2015 G2 (MASTER) is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2015 G2 (MASTER) 06h31m10s 13°30'S 6.5

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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