|
58P/Jackson-Neujmin |
| ephemeris |
date |
magn |
radius |
delta |
ra |
dec |
elong |
phase |
PA |
| Today | 10 Apr 2026 | 39.9 | 5.919 AU | 4.932 AU td > | 13h35m | +01°31' | 169.2° | 1.8° | 209° |
| Perihelion | 4 Sep 2028 | 7.6 | 1.386 AU | 0.526 AU td > | 02h25m | +01°40' | 126.2° | 36.0° | 260° |
| Nearest approach | 21 Sep 2028 | 7.7 | 1.401 AU | 0.509 AU td > | 03h02m | -04°01' | 133.0° | 31.6° | 273° |
58P/Jackson-Neujmin- 2026-04-10
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 2.9 + 5 log[∆] + 43.4 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 58P/Jackson-Neujmin are:
e (Eccentricity) : 0.6613140
q (Perihelion distance) : 1.3859630
i (Inclination) : 13.08270
Ω (Longitude of ascending node) : 159.02330
ω (Argument of perihelion) : 200.57520
L (Longitude of perihelion) : 179.10764
B (Latitude of perihelion) : -4.56271
T (Time of perihelion passage) : 2462018.73770
P (Orbital period in years) : 8.28
Epoch : 2026 Apr 09
Reference : MPC191597
Classification(s): : Ecliptic; Jupiter family
Tisserand (Jupiter) : 2.567
Ephemerides
Date Time RA (2000) DEC (2000) delta radius elong phase PA magn
2026-04-09 00:00 UT 13 36 26.3 +01 25 20 4.938 5.923 168.9 1.9 217 39.9
2026-04-10 00:00 UT 13 35 54.3 +01 29 17 4.934 5.920 169.2 1.8 212 39.9
2026-04-10 11:50 UT 13 35 38.4 +01 31 13 4.932 5.919 169.2 1.8 209 39.9
2026-04-11 00:00 UT 13 35 22.1 +01 33 12 4.930 5.918 169.3 1.8 206 39.8
2026-04-12 00:00 UT 13 34 49.8 +01 37 05 4.927 5.915 169.3 1.8 200 39.8
2026-04-13 00:00 UT 13 34 17.4 +01 40 57 4.924 5.912 169.2 1.8 194 39.8
2026-04-14 00:00 UT 13 33 45.0 +01 44 46 4.922 5.909 169.0 1.9 188 39.8
2026-04-15 00:00 UT 13 33 12.4 +01 48 33 4.919 5.906 168.6 1.9 182 39.8
2026-04-16 00:00 UT 13 32 39.9 +01 52 18 4.918 5.903 168.2 2.0 177 39.8
2026-04-17 00:00 UT 13 32 07.3 +01 56 01 4.916 5.900 167.7 2.1 172 39.8
2026-04-18 00:00 UT 13 31 34.7 +01 59 41 4.915 5.897 167.1 2.2 168 39.8
2026-04-19 00:00 UT 13 31 02.1 +02 03 18 4.914 5.894 166.4 2.3 164 39.8
2026-04-20 00:00 UT 13 30 29.6 +02 06 53 4.913 5.892 165.7 2.4 160 39.8
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.