|
C/2020 K8 (Catalina-ATLAS) |
| ephemeris |
date |
magn |
radius |
delta |
ra |
dec |
elong |
phase |
PA |
| Nearest approach | 15 Aug 2020 | 14.9 | 0.871 AU | 0.573 AU td > | 05h31m | +27°00' | 59.2° | 86.4° | 269° |
| Perihelion | 15 Sep 2020 | 15.5 | 0.473 AU | 1.090 AU td > | 09h53m | -00°49' | 25.7° | 67.2° | 262° |
| Today | 19 Jul 2026 | 26.0 | 17.791 AU | 17.326 AU td > | 15h58m | +08°04' | 115.7° | 3.0° | 118° |
C/2020 K8 (Catalina-ATLAS)- 2026-07-19
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 16.2 + 5 log[∆] + 2.9 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 K8 (Catalina-ATLAS) are:
e (Eccentricity) : 1.0003650
q (Perihelion distance) : 0.4731330
i (Inclination) : 31.29930
Ω (Longitude of ascending node) : 181.12570
ω (Argument of perihelion) : 260.35640
L (Longitude of perihelion) : 259.87851
B (Latitude of perihelion) : -30.80831
T (Time of perihelion passage) : 2459108.38430
Epoch : 2026 May 29
Reference : MPC194168
Classification(s): : Nearly isotropic; New (a > 10000 AU)
Ephemerides
Date Time RA (2000) DEC (2000) delta radius elong phase PA magn
2026-07-18 00:00 UT 15 58 45.1 +08 06 03 17.305 17.784 116.6 2.9 119 26.0
2026-07-19 00:00 UT 15 58 38.2 +08 05 05 17.324 17.790 115.8 2.9 118 26.0
2026-07-19 03:09 UT 15 58 37.4 +08 04 58 17.326 17.791 115.7 3.0 118 26.0
2026-07-20 00:00 UT 15 58 31.6 +08 04 06 17.342 17.796 115.0 3.0 117 26.0
2026-07-21 00:00 UT 15 58 25.1 +08 03 05 17.361 17.801 114.1 3.0 117 26.0
2026-07-22 00:00 UT 15 58 18.8 +08 02 04 17.380 17.807 113.3 3.0 116 26.0
2026-07-23 00:00 UT 15 58 12.8 +08 01 00 17.400 17.813 112.4 3.0 116 26.0
2026-07-24 00:00 UT 15 58 06.9 +07 59 56 17.419 17.819 111.6 3.0 115 26.0
2026-07-25 00:00 UT 15 58 01.3 +07 58 51 17.438 17.824 110.8 3.1 115 26.0
2026-07-26 00:00 UT 15 57 55.8 +07 57 44 17.458 17.830 109.9 3.1 114 26.0
2026-07-27 00:00 UT 15 57 50.6 +07 56 36 17.477 17.836 109.1 3.1 114 26.0
2026-07-28 00:00 UT 15 57 45.6 +07 55 27 17.497 17.841 108.2 3.1 113 26.1
2026-07-29 00:00 UT 15 57 40.7 +07 54 17 17.517 17.847 107.4 3.1 113 26.1
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.