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

Comet C/2018 W1 (Catalina) passes perihelion

Dominic Ford, Editor
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Comet C/2018 W1 (Catalina) will make its closest approach to the Sun on 12 May, at a distance of 1.36 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 30° below the horizon at dusk.

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The events that comprise the 2019 apparition of C/2018 W1 (Catalina) are as follows:

Date Event
12 May 2019Comet C/2018 W1 (Catalina) passes perihelion

The table below lists the times when C/2018 W1 (Catalina) will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
21 Apr 2019EridanusNot observable
23 Apr 2019EridanusNot observable
25 Apr 2019EridanusNot observable
27 Apr 2019EridanusNot observable
29 Apr 2019EridanusNot observable
01 May 2019EridanusNot observable
03 May 2019EridanusNot observable
05 May 2019EridanusNot observable
07 May 2019EridanusNot observable
09 May 2019EridanusNot observable
11 May 2019EridanusNot observable
13 May 2019EridanusNot observable
15 May 2019EridanusNot observable
17 May 2019EridanusNot observable
19 May 2019EridanusNot observable
21 May 2019EridanusNot observable
23 May 2019EridanusNot observable
25 May 2019LepusNot observable
27 May 2019LepusNot observable
29 May 2019LepusNot observable
31 May 2019ColumbaNot observable

A more detailed table of C/2018 W1 (Catalina)'s position on each night is available here. A diagram of the orbit of C/2018 W1 (Catalina) is available here.

Finder chart

The chart below shows the path of C/2018 W1 (Catalina) 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/2018 W1 (Catalina) is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet C/2018 W1 (Catalina) 04h18m40s 20°42'S Eridanus 11.4

The coordinates are given in J2000.0.

The sky on 12 May 2019

The sky on 12 May 2019
Sunrise
05:24
Sunset
19:55
Twilight ends
21:52
Twilight begins
03:28

8-day old moon
Waxing Gibbous

62%

8 days old

Planets
Rise Culm. Set
Mercury 05:04 12:00 18:56
Venus 04:29 11:04 17:39
Moon 12:40 19:52 02:52
Mars 07:30 15:12 22:54
Jupiter 22:18 02:53 07:27
Saturn 00:12 04:51 09:30
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 02 Jan 2024.

Image credit

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

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Cambridge

Latitude:
Longitude:
Timezone:

42.38°N
71.11°W
EDT

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