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

C/2013 V5 (Oukaimeden) reaches its brightest

Dominic Ford, Editor
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Comet C/2013 V5 (Oukaimeden) is forecast to reach its brightest. It will lie at a distance of 0.66 AU from the Sun, and at a distance of 0.48 AU from the Earth.

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

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Based on the absolute magnitude published for this comet by the British Astronomical Association's Comet Section, we estimate that it may reach a peak brightness of around mag 6.

This comet is not expected to be visible to the naked eye, but might be visible through bird-watching binoculars. The brightnesses of comets are often highly unpredictable, since it is impossible to predict with certainty how they will respond as they are heated by the Sun as they move into the inner solar system. Magnitude estimates should be assumed to be highly provisional more than a few weeks in advance.

The path of the comet, on the other hand, can reliably be predicted. The chart below shows the path of C/2013 V5 (Oukaimeden) over the course of its apparition. It was produced using StarCharter and 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.

Alternatively, you can create a textual listing of the comet's position using In-The-Sky.org's ephemeris generator.

The position of comet C/2013 V5 (Oukaimeden) at its brightest will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2013 V5 (Oukaimeden) 10h59m30s -30°37' Hydra 6.2

The coordinates are given in J2000.0.

The sky on 16 September 2014
Twilight ends
Twilight begins

22-day old moon
Waning Crescent


22 days old

Rise Culm. Set
Mercury 08:42 14:10 19:38
Venus 05:31 12:03 18:35
Moon 23:37 06:52 14:06
Mars 12:21 16:58 21:36
Jupiter 02:55 10:05 17:15
Saturn 11:05 16:10 21:14
All times shown in EDT.


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 20 Aug 2019.

Image credit

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




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