Sidereal Orbital Period of Neptune

TNeptune=5,200,329,600 sT_{\mathrm{Neptune}} = 5,200,329,600\ \text{s}
Value5,200,329,600 s
StatusConventional / typical value
SourceNASA NSSDC Planetary Fact Sheet, Neptune (sidereal orbit period)
CategoriesAstronomicalsolar-systemplanets
Sidereal Orbital Period of Neptune in every time unit
Planck time9.6458752e+52 tP
attosecond5.2003296e+27 as
femtosecond5.2003296e+24 fs
picosecond5.2003296e+21 ps
nanosecond5.2003296e+18 ns
shake5.2003296e+17 shake
microsecond5.2003296e+15 μs
millisecond5,200,329,600,000 ms
second5,200,329,600 s
minute86,672,160 min
hour1,444,536 h
sidereal day60,353.792 sd
day60,189 d
week8,598.4286 wk
fortnight4,299.2143 fn
month1,977.5026 mo
year164.7885 yr
decade16.47885 dec
century1.647885 cent
millennium0.1647885 mil
megayear0.0001647885 Myr
eon1.6478850e-07 eon

Learning zone

Neptune's year is so long that the planet has been observed for barely one of them: discovered on 23 September 1846, it returned to the same heliocentric longitude on 11 July 2011, having completed a single circuit while Earth ran 165. Every claim about long-term behaviour — seasonal change, cloud cycles, the waxing of southern summer since Voyager — rests on less than one Neptunian year of data, most of it from Earth-based telescopes and Hubble.

The period's most elegant service predates the discovery itself. Le Verrier's computed orbit, fed to Galle with a position good to one degree, implicitly contained this period through Kepler's third law; the actual 164.8-year figure emerged within months once pre-discovery sightings were recognised — including Galileo's, who plotted Neptune as a fixed star near Jupiter in December 1612 and January 1613, and even noted that it seemed to have moved. He was one careful night from finding a planet 233 years early.