47171 Lempo

47171 Lempo
Lempo–Hiisi and their outer companion Paha, imaged with the Hubble Space Telescope in 2001. Lempo and Hiisi are unresolved.
Discovery
Discovered byEric P. Rubenstein
Louis-Gregory Strolger
Discovery siteKitt Peak National Obs.
Discovery date1 October 1999
Designations
(47171) Lempo
Pronunciation/ˈlɛmp/
Named after
Lempo (Finnish mythology)
1999 TC36
TNO · plutino · distant · triple
Orbital characteristics
Epoch 17 December 2020 (JD 2459200.5)
Uncertainty parameter 1
Observation arc46.58 yr (17,013 days)
Earliest precovery date18 June 1974
Aphelion48.397 AU
Perihelion30.542 AU
39.470 AU
Eccentricity0.22618
247.97 yr (90,572 days)
8.547°
0° 0m 14.309s / day
Inclination8.4233°
97.020°
294.424°
Known satellites2
Physical characteristics
272+17
−19
 km
(primary)
Mass(12.75±0.06)×1018 kg
(overall system)
(14.20±0.05)×1018 kg
(without Paha)
6.71×1018 kg
(primary)
Mean density
0.64+0.15
−0.11
 g/cm3
 (system)
0.079+0.013
−0.011
 (system)
RR (very red)
B–V=1.029±0.047
V−R=0.693±0.032
V−I=1.270±0.050
19.9
5.41±0.10
4.8 (assumed)

    47171 Lempo, or as a binary (47171) Lempo–Hiisi (provisional designation 1999 TC36), is a triple trans-Neptunian object in the Kuiper belt, located in the outermost regions of the Solar System. It was discovered on 1 October 1999, by American astronomers Eric Rubenstein and Louis-Gregory Strolger during an observing run at Kitt Peak National Observatory in Arizona, United States. Rubenstein was searching images taken by Strolger as part of their Nearby Galaxies Supernova Search project. It is classified as a plutino with a 2:3 mean-motion resonance with Neptune and is among the brighter TNOs. It reached perihelion in July 2015. This minor planet was named after Lempo from Finnish mythology.

    The system's other two components, Paha /ˈpɑːhɑː/ and Hiisi /ˈhsi/, were discovered in 2001 and 2007, respectively, and later named after Lempo's two demon cohorts, Paha and Hiisi.