C/2025 L2 |
ephemeris |
date |
magn |
radius |
delta |
ra |
dec |
elong |
phase |
PA |
Today | 13 Jun 2025 | 19.4 | 3.420 AU | 2.917 AU | 22h20m | -15°18' | 111.3° | 16.1° | 251° |
Nearest approach | 14 Aug 2025 | 18.3 | 3.119 AU | 2.182 AU | 21h40m | -41°04' | 153.2° | 8.4° | 357° |
Perihelion | 19 Dec 2025 | 18.8 | 2.835 AU | 3.335 AU | 21h23m | -60°27' | 51.8° | 15.8° | 111° |
C/2025 L2- 2025-06-13
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.)
The orbital elements of C/2025 L2 are:
e (Eccentricity) : 1.0150730
q (Perihelion distance) : 2.8346220
i (Inclination) : 86.71700
Ω (Longitude of ascending node) : 135.03240
ω (Argument of perihelion) : 232.62790
L (Longitude of perihelion) : 139.32035
B (Latitude of perihelion) : -52.50496
T (Time of perihelion passage) : 2461029.48140
Epoch : 2025 Jun 12
Reference : MPEC 2025-L62
Classification(s): : Nearly isotropic; New (a > 10000 AU)
The light curve chart below shows the estimated development of the comet's magnitude. Blue and black dots are visual and photometric CCD observations respectively from COBS or the MPC.
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. (11.70 + 5 log[∆] + 10.00 log[r]).
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.
A more printer-friendly version of the same chart can be found further down this page as well.
The following chart shows the current location of the comet in a smaller, upside-down telescopic field of view.
A printable version of the short-term path of the comet in a field of view that is optimized for (~10x50) binoculars and finderscopes.
Ephemerides:
Date Time RA (2000) DEC (2000) delta radius elong phase PA magn
2025-06-13 00:00 UT 22 20 11.4 -15 04 06 2.936 3.425 110.4 16.1 250 19.4
2025-06-13 21:14 UT 22 20 17.8 -15 18 17 2.917 3.420 111.3 16.1 251 19.4
2025-06-14 00:00 UT 22 20 18.6 -15 20 09 2.915 3.419 111.4 16.0 251 19.4
2025-06-15 00:00 UT 22 20 24.7 -15 36 32 2.894 3.414 112.5 16.0 251 19.3
2025-06-16 00:00 UT 22 20 29.7 -15 53 15 2.874 3.408 113.5 15.9 251 19.3
2025-06-17 00:00 UT 22 20 33.6 -16 10 19 2.854 3.403 114.5 15.8 251 19.3
2025-06-18 00:00 UT 22 20 36.4 -16 27 43 2.834 3.398 115.5 15.7 251 19.3
2025-06-19 00:00 UT 22 20 37.9 -16 45 27 2.814 3.392 116.6 15.5 252 19.3
2025-06-20 00:00 UT 22 20 38.3 -17 03 33 2.794 3.387 117.6 15.4 252 19.2
2025-06-21 00:00 UT 22 20 37.5 -17 21 60 2.774 3.381 118.7 15.3 252 19.2
2025-06-22 00:00 UT 22 20 35.4 -17 40 48 2.755 3.376 119.7 15.2 253 19.2
2025-06-23 00:00 UT 22 20 32.0 -17 59 57 2.736 3.371 120.8 15.0 253 19.2
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.