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

Comet 2P/Encke passes perigee

Dominic Ford, Editor
From the Comets feed

Objects: 2P/Encke
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The sky at

Comet 2P/Encke will make its closest approach to the Earth on 17 March, at a distance of of 0.65 AU.

From Cambridge on the day of perigee it will not be readily observable since it will be very close to the Sun, at a separation of only 4° from it.

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The events that comprise the 2017 apparition of 2P/Encke are as follows:

Date Event
14 Mar 2017Comet 2P/Encke passes perihelion
17 Mar 2017Comet 2P/Encke passes perigee

The table below lists the times when 2P/Encke will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
24 Feb 2017PiscesNot observable
26 Feb 2017PiscesNot observable
28 Feb 2017PiscesNot observable
02 Mar 2017PiscesNot observable
04 Mar 2017PiscesNot observable
06 Mar 2017PiscesNot observable
08 Mar 2017PiscesNot observable
10 Mar 2017PiscesNot observable
12 Mar 2017PiscesNot observable
14 Mar 2017PiscesNot observable
16 Mar 2017AquariusNot observable
18 Mar 2017AquariusNot observable
20 Mar 2017AquariusNot observable
22 Mar 2017AquariusNot observable
24 Mar 2017AquariusNot observable
26 Mar 2017AquariusNot observable
28 Mar 2017AquariusNot observable
30 Mar 2017AquariusNot observable
01 Apr 2017AquariusNot observable
03 Apr 2017AquariusNot observable
05 Apr 2017AquariusNot observable

A more detailed table of 2P/Encke's position on each night is available here. A diagram of the orbit of 2P/Encke is available here.

Finder chart

The chart below shows the path of 2P/Encke 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 2P/Encke is currently available.

The comet's position at perigee will be:

Object Right Ascension Declination Constellation Magnitude
Comet 2P/Encke 23h39m20s 5°34'S Aquarius 5.0

The coordinates are given in J2000.0.

The sky on 17 Mar 2017

The sky on 17 March 2017
Sunrise
06:50
Sunset
18:53
Twilight ends
20:27
Twilight begins
05:16

19-day old moon
Waning Gibbous

72%

19 days old

Planets
Rise Culm. Set
Mercury 07:16 13:29 19:42
Venus 06:37 13:23 20:08
Moon 23:02 04:21 09:35
Mars 08:19 15:13 22:07
Jupiter 20:43 02:22 08:01
Saturn 02:15 06:51 11:28
All times shown in EDT.

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 10 Dec 2024.

Image credit

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

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Cambridge

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42.38°N
71.11°W
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