|
P/2020 U2 (PANSTARRS) |
| ephemeris |
date |
magn |
radius |
delta |
ra |
dec |
elong |
phase |
PA |
| Today | 30 May 2026 | 22.6 | 4.734 AU | 3.958 AU td > | 19h43m | -27°56' | 135.5° | 8.6° | 267° |
| Nearest approach | 22 Sep 2027 | 18.2 | 2.626 AU | 1.669 AU td > | 22h31m | -08°53' | 157.7° | 8.3° | 69° |
| Perihelion | 1 May 2028 | 17.8 | 1.847 AU | 2.784 AU td > | 03h40m | +23°55' | 17.4° | 9.4° | 63° |
P/2020 U2 (PANSTARRS)- 2026-05-30
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 12.9 + 5 log[∆] + 10.0 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 P/2020 U2 (PANSTARRS) are:
e (Eccentricity) : 0.5111450
q (Perihelion distance) : 1.8467140
i (Inclination) : 6.41880
Ω (Longitude of ascending node) : 342.77070
ω (Argument of perihelion) : 84.83130
L (Longitude of perihelion) : 67.56957
B (Latitude of perihelion) : 6.39259
T (Time of perihelion passage) : 2461893.28380
P (Orbital period in years) : 7.34
Epoch : 2026 May 29
Reference : MPC194170
Classification(s): : Ecliptic; Jupiter family
Tisserand (Jupiter) : 2.833
Ephemerides
Date Time RA (2000) DEC (2000) delta radius elong phase PA magn
2026-05-29 00:00 UT 19 44 30.6 -27 54 18 3.980 4.739 133.9 8.9 266 22.7
2026-05-30 00:00 UT 19 44 10.6 -27 55 57 3.966 4.736 134.9 8.7 266 22.6
2026-05-30 13:36 UT 19 43 58.8 -27 56 54 3.958 4.734 135.5 8.6 267 22.6
2026-05-31 00:00 UT 19 43 49.6 -27 57 38 3.952 4.733 135.9 8.6 267 22.6
2026-06-01 00:00 UT 19 43 27.7 -27 59 19 3.938 4.730 136.9 8.4 267 22.6
2026-06-02 00:00 UT 19 43 04.8 -28 01 01 3.925 4.727 138.0 8.3 267 22.6
2026-06-03 00:00 UT 19 42 41.0 -28 02 45 3.911 4.724 139.0 8.1 268 22.6
2026-06-04 00:00 UT 19 42 16.3 -28 04 29 3.898 4.720 140.0 7.9 268 22.6
2026-06-05 00:00 UT 19 41 50.7 -28 06 14 3.885 4.717 141.1 7.8 268 22.6
2026-06-06 00:00 UT 19 41 24.2 -28 07 60 3.872 4.714 142.1 7.6 269 22.6
2026-06-07 00:00 UT 19 40 56.7 -28 09 46 3.859 4.711 143.2 7.4 269 22.6
2026-06-08 00:00 UT 19 40 28.4 -28 11 33 3.847 4.708 144.2 7.2 270 22.6
2026-06-09 00:00 UT 19 39 59.3 -28 13 20 3.835 4.705 145.2 7.1 270 22.5
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.