|
C/2020 W5 (Lemmon) |
| ephemeris |
date |
magn |
radius |
delta |
ra |
dec |
elong |
phase |
PA |
| Perihelion | 1 Dec 2020 | 22.3 | 3.372 AU | 2.519 AU td > | 04h55m | +56°44' | 144.7° | 9.7° | 191° |
| Nearest approach | 1 Dec 2020 | 22.3 | 3.372 AU | 2.519 AU td > | 04h53m | +56°57' | 144.8° | 9.7° | 188° |
| Today | 9 Dec 2025 | 32.3 | 13.913 AU | 14.734 AU td > | 17h07m | +09°33' | 32.4° | 2.2° | 2° |
C/2020 W5 (Lemmon)- 2025-12-09
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.
The light curve is based on the absolute magnitude and slope parameter as calculated from an MPEC, or the latest values provided by the minor planet center. (15.0 + 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 C/2020 W5 (Lemmon) are:
e (Eccentricity) : 1.0023490
q (Perihelion distance) : 3.3721600
i (Inclination) : 88.61020
Ω (Longitude of ascending node) : 75.47100
ω (Argument of perihelion) : 24.62830
L (Longitude of perihelion) : 76.10804
B (Latitude of perihelion) : 24.62057
T (Time of perihelion passage) : 2459184.59560
Epoch : 2025 Nov 12
Reference : MPEC 2021-BE3
Classification(s): : Nearly isotropic; New (a > 10000 AU)
Ephemerides
Date Time RA (2000) DEC (2000) delta radius elong phase PA magn
2025-12-08 00:00 UT 17 07 25.9 +09 34 22 14.728 13.906 32.3 2.2 4 32.3
2025-12-09 00:00 UT 17 07 42.1 +09 33 19 14.733 13.911 32.4 2.2 2 32.3
2025-12-09 04:45 UT 17 07 45.3 +09 33 07 14.734 13.913 32.4 2.2 2 32.3
2025-12-10 00:00 UT 17 07 58.3 +09 32 18 14.738 13.917 32.4 2.2 0 32.3
2025-12-11 00:00 UT 17 08 14.5 +09 31 19 14.743 13.923 32.5 2.2 359 32.3
2025-12-12 00:00 UT 17 08 30.7 +09 30 23 14.747 13.929 32.6 2.2 357 32.3
2025-12-13 00:00 UT 17 08 46.9 +09 29 29 14.752 13.934 32.7 2.2 355 32.3
2025-12-14 00:00 UT 17 09 03.1 +09 28 37 14.756 13.940 32.9 2.2 353 32.3
2025-12-15 00:00 UT 17 09 19.2 +09 27 47 14.760 13.946 33.1 2.2 352 32.3
2025-12-16 00:00 UT 17 09 35.3 +09 26 60 14.763 13.951 33.3 2.2 350 32.3
2025-12-17 00:00 UT 17 09 51.4 +09 26 15 14.767 13.957 33.5 2.2 348 32.3
2025-12-18 00:00 UT 17 10 07.4 +09 25 32 14.770 13.963 33.7 2.2 347 32.3
2025-12-19 00:00 UT 17 10 23.4 +09 24 52 14.773 13.968 34.0 2.3 345 32.3
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.