Comet C/2013 X1 (PANSTARRS) reaches peak brightness

Dominic Ford, Editor
From the Comets feed


Comet C/2013 X1 (PANSTARRS) is forecast to reach the brightest point in its 2016 apparition on 17 June. At that time, it will lie at a distance of 1.58 AU from the Sun, and at a distance of 0.68 AU from the Earth.

From Cambridge on 17 June it will not be readily observable since it will lie so far south that it will never rise more than 7° above the horizon.

The events that comprise the 2016 apparition of C/2013 X1 (PANSTARRS) are as follows:

Date Event
20 Apr 2016Comet C/2013 X1 (PANSTARRS) passes perihelion
17 Jun 2016Comet C/2013 X1 (PANSTARRS) reaches peak brightness
21 Jun 2016Comet C/2013 X1 (PANSTARRS) passes perigee

The table below lists the times when C/2013 X1 (PANSTARRS) will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
27 May 2016AquariusNot observable
29 May 2016AquariusNot observable
31 May 2016AquariusNot observable
02 Jun 2016AquariusNot observable
04 Jun 2016AquariusNot observable
06 Jun 2016AquariusNot observable
08 Jun 2016Piscis AustrinusNot observable
10 Jun 2016Piscis AustrinusNot observable
12 Jun 2016Piscis AustrinusNot observable
14 Jun 2016MicroscopiumNot observable
16 Jun 2016MicroscopiumNot observable
18 Jun 2016SagittariusNot observable
20 Jun 2016SagittariusNot observable
22 Jun 2016TelescopiumNot observable
24 Jun 2016TelescopiumNot observable
26 Jun 2016TelescopiumNot observable
28 Jun 2016AraNot observable
30 Jun 2016AraNot observable
02 Jul 2016AraNot observable
04 Jul 2016NormaNot observable
06 Jul 2016NormaNot observable

A more detailed table of C/2013 X1 (PANSTARRS)'s position on each night is available here. A diagram of the orbit of C/2013 X1 (PANSTARRS) is available here.

Finder chart

The chart below shows the path of C/2013 X1 (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/2013 X1 (PANSTARRS) is currently available.

The comet's position on 17 June 2016 will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2013 X1 (PANSTARRS) 20h47m50s 40°03'S Microscopium 6.0

The coordinates are given in J2000.0.

The sky on 17 Jun 2016

The sky on 17 June 2016
Sunrise
05:04
Sunset
20:24
Twilight ends
22:39
Twilight begins
02:49


Waxing Gibbous

94%

12 days old

Planets
Rise Culm. Set
Mercury 04:01 11:20 18:38
Venus 05:18 12:57 20:35
Moon 17:46 22:54 03:58
Mars 17:39 22:20 03:02
Jupiter 11:36 18:05 00:34
Saturn 18:55 23:39 04:23
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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