Comet 41P/Tuttle-Giacobini-Kresak will make its closest approach to the Sun, at a distance of 1.05 AU.
|25 Mar 2017||–||41P/Tuttle-Giacobini-Kresak at perigee|
|31 Mar 2017||–||41P/Tuttle-Giacobini-Kresak reaches its brightest|
|10 Apr 2017||–||41P/Tuttle-Giacobini-Kresak at perihelion|
|20 Mar 2017||Canes Venatici||Visible from 20:10 until 05:49|
Highest at 02:24, 83° above N horizon
|22 Mar 2017||Ursa Major||Visible from 20:12 until 05:45|
Highest at 02:42, 82° above N horizon
|24 Mar 2017||Bootes||Visible from 20:15 until 05:42|
Highest at 03:01, 81° above N horizon
|26 Mar 2017||Bootes||Visible from 20:17 until 05:38|
Highest at 03:21, 80° above N horizon
|28 Mar 2017||Bootes||Visible from 20:29 until 05:35|
Highest at 03:41, 80° above N horizon
|30 Mar 2017||Bootes||Visible from 20:50 until 05:31|
Highest at 03:59, 81° above N horizon
|01 Apr 2017||Hercules||Visible from 21:11 until 05:27|
Highest at 04:15, 82° above N horizon
|03 Apr 2017||Hercules||Visible from 21:31 until 05:24|
Highest at 04:29, 83° above N horizon
|05 Apr 2017||Hercules||Visible from 21:50 until 05:20|
Highest at 04:41, 84° above N horizon
|07 Apr 2017||Hercules||Visible from 22:07 until 05:17|
Highest at 04:50, 86° above N horizon
|09 Apr 2017||Hercules||Visible from 22:22 until 05:13|
Highest at 04:58, 87° above N horizon
|11 Apr 2017||Hercules||Visible from 22:35 until 05:09|
Highest at 05:03, 89° above N horizon
|13 Apr 2017||Hercules||Visible from 22:45 until 05:06|
Highest at 05:06, 90° above SE horizon
|15 Apr 2017||Hercules||Visible from 22:54 until 05:02|
Highest at 05:02, 88° above SE horizon
|17 Apr 2017||Hercules||Visible from 23:01 until 04:59|
Highest at 04:59, 86° above SE horizon
|19 Apr 2017||Hercules||Visible from 23:06 until 04:55|
Highest at 04:55, 84° above SE horizon
|21 Apr 2017||Lyra||Visible from 23:11 until 04:52|
Highest at 04:52, 82° above SE horizon
|23 Apr 2017||Lyra||Visible from 23:14 until 04:48|
Highest at 04:48, 81° above SE horizon
|25 Apr 2017||Lyra||Visible from 23:16 until 04:45|
Highest at 04:45, 80° above SE horizon
|27 Apr 2017||Lyra||Visible from 23:17 until 04:42|
Highest at 04:42, 78° above SE horizon
|29 Apr 2017||Lyra||Visible from 23:18 until 04:38|
Highest at 04:38, 77° above S horizon
At the moment of perihelion it will be visible in the morning sky, becoming accessible around 22:18, when it reaches an altitude of 21° above your north-eastern horizon. It will then reach its highest point in the sky at 04:54, 86° above your northern horizon. It will be lost to dawn twilight around 05:11, 85° above your north-western horizon.
The chart below shows the path of 41P/Tuttle-Giacobini-Kresak 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.
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 41P/Tuttle-Giacobini-Kresak is currently available.
The comet's position at perihelion will be:
The coordinates are given in J2000.0.
|The sky on 10 April 2017|
13 days old
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 27 Dec 2021.
© Andy Roberts 1997. Pictured comet is C/1995 O1 Hale-Bopp.