C/2017 T2 (PANSTARRS) |
ephemeris |
date |
magn |
radius |
delta |
ra |
dec |
elong |
phase |
PA |
Nearest approach | 28 Dec 2019 | 9.8 | 2.334 AU | 1.524 AU | 03h34m | +52°51' | 136.0° | 17.0° | 115° |
Perihelion | 6 May 2020 | 8.6 | 1.603 AU | 1.699 AU | 07h01m | +75°32' | 67.1° | 35.4° | 67° |
Today | 16 Oct 2025 | 22.3 | 15.938 AU | 16.097 AU | 19h00m | -66°36' | 79.1° | 3.5° | 92° |
C/2017 T2 (PANSTARRS)- 2025-10-16
astro.vanbuitenen.nl
The interactive orbit chart above shows the comet's path through the solar system and its position at the given date.
Green and blue lines are shown perpendicular to the ecliptic plane: Green if the path is above the ecliptic plane, blue if it is below.
(Left-click and drag to rotate the view; Right-click and drag to move the view; Use scroll wheel to zoom in our out.)
Light curve
The light curve chart below shows the estimated development of the comet's magnitude. Blue and black dots are visual and photometric CCD observations from COBS.
This lightcurve is being recalculated every 6 hours based on the available COBS/MPC observations (currently 5.7 + 5 log[∆] + 8.8 log[r]). An additional green curve is displayed when an increase in apparent brightness is expected due to forward scattering of sunlight, which occurs when a dust-rich comet is located between the Earth and the Sun. (See Marcus 2007)
Charts
The all-sky chart below shows the path of the comet over the same period as the light curve. The comet's current position is marked yellow.
The following chart shows the short-term path of the comet in a field of view that is optimized for (~10x50) binoculars and finderscopes.
Orbital elements
The orbital elements of C/2017 T2 (PANSTARRS) are:
e (Eccentricity) : 0.9990290
q (Perihelion distance) : 1.6025270
i (Inclination) : 57.27700
Ω (Longitude of ascending node) : 64.42410
ω (Argument of perihelion) : 92.77200
L (Longitude of perihelion) : -20.45771
B (Latitude of perihelion) : 57.17281
T (Time of perihelion passage) : 2458975.83810
P (Orbital period in years) : 67046.97
Epoch : 2025 Oct 15
Reference : MPEC 2024-A43
Classification(s): : Nearly isotropic; Returning (a < 10000 AU); External (P > 200 years)
Ephemerides
Date Time RA (2000) DEC (2000) delta radius elong phase PA magn
2025-10-15 00:00 UT 18 59 53.2 -66 40 56 16.064 15.927 80.3 3.5 91 22.2
2025-10-16 00:00 UT 19 00 03.2 -66 38 36 16.081 15.933 79.7 3.5 92 22.2
2025-10-16 20:51 UT 19 00 12.3 -66 36 36 16.097 15.938 79.1 3.5 92 22.3
2025-10-17 00:00 UT 19 00 13.8 -66 36 17 16.099 15.939 79.0 3.5 93 22.3
2025-10-18 00:00 UT 19 00 24.9 -66 33 59 16.117 15.945 78.3 3.5 93 22.3
2025-10-19 00:00 UT 19 00 36.7 -66 31 40 16.134 15.950 77.6 3.5 94 22.3
2025-10-20 00:00 UT 19 00 49.0 -66 29 23 16.152 15.956 76.9 3.5 94 22.3
2025-10-21 00:00 UT 19 01 01.8 -66 27 05 16.169 15.962 76.2 3.5 95 22.3
2025-10-22 00:00 UT 19 01 15.2 -66 24 49 16.187 15.968 75.5 3.5 96 22.3
2025-10-23 00:00 UT 19 01 29.2 -66 22 33 16.204 15.973 74.8 3.4 96 22.3
2025-10-24 00:00 UT 19 01 43.6 -66 20 17 16.221 15.979 74.2 3.4 97 22.3
2025-10-25 00:00 UT 19 01 58.6 -66 18 02 16.239 15.985 73.5 3.4 98 22.3
2025-10-26 00:00 UT 19 02 14.2 -66 15 48 16.256 15.991 72.8 3.4 99 22.3
Terminology:
delta: distance between comet and earth in AU
radius: distance between comet and sun in AU
magn: magnitude (brightness) estimate
ra: right ascension in hours (24h = 360deg)
dec: declination in degrees
elong: elongation in degrees (angle sun-earth-comet)
phase: phase angle in degrees (angle sun-comet-earth)
AU: Astronomical Unit (mean distance between earth and sun: 149597870.7 km
Orbital elements usually provided by the MPC (Minor Planet Center).
Observations contributed by observers worldwide, via COBS (Comet Observation Database) or the MPC (Minor Planet Center)
Calculations by a modified version of AAPlus, a C# implementation of the AA+ project by PJ Naughter from the algorithms presented in the book "Astronomical Algorithms" by Jean Meeus.
NGC2000 dso catalog and star labels from VizieR as provided by the Strasbourg astronomical Data Center.
Tycho2 catalog from the ESO archive.