Comet C/2017 T2 (PANSTARRS) is forecast to reach its brightest. It will lie at a distance of 1.62 AU from the Sun, and at a distance of 1.67 AU from the Earth.

From Fairfield the 2020 apparition of C/2017 T2 (PANSTARRS) will progress as follows:

A more detailed table of C/2017 T2 (PANSTARRS)'s position on each night is available here. A diagram of the orbit of C/2017 T2 (PANSTARRS) is available here.

On 14 May it will be very well placed – it will be close enough to the north celestial pole that it will be high above the horizon all night.

Finder chart

The chart below shows the path of C/2017 T2 (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.

Click to expand »

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 For most comets, we do not publish any magnitude estimates at all.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.

Based on the magnitude parameters published for this comet by the BAA Comet Section, we estimate that it may be around mag 9 on 14 May 2020. This estimate is based on observations that the BAA has received from amateur astronomers, assuming that its current level of activity will remain constant.

This comet is not expected to be visible to the naked eye, but might be visible through bird-watching binoculars.

The comet's position on 14 May 2020 will be:

The coordinates are given in J2000.0.

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 15 Jan 2021.

Image credit

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

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