Back (41) Daphne ALS 41 دافني Arabic 41 دافني (كويكب) ARZ 41 Daphne AST (41) Дафна Byelorussian (41) Dafne Catalan (41) Дафна CE Daphne (planetka) Czech (41) Daphne German 41 Δάφνη Greek
 | |
| Discovery[1] | |
|---|---|
| Discovered by | H. Goldschmidt |
| Discovery date | May 22, 1856 |
| Designations | |
| (41) Daphne | |
| Pronunciation | /ˈdæfni/[2] |
Named after | Daphnē |
| 1949 TG | |
| Main belt | |
| Adjectives | Daphnean /ˈdæfniən/[3] |
| Orbital characteristics[1] | |
| Epoch 31 December 2006 (JD 2454100.5) | |
| Aphelion | 3.517 AU (526.144 Gm) |
| Perihelion | 2.014 AU (301.220 Gm) |
| 2.765 AU (413.682 Gm) | |
| Eccentricity | 0.272 |
| 4.60 a (1,679.618 d) | |
| 247.500° | |
| Inclination | 15.765° |
| 178.159° | |
| 46.239° | |
| Known satellites | Peneius /pɛˈniːəs/ (S/2008 (41) 1) |
| Physical characteristics | |
| Dimensions | 213×160 km[4] 239x183x153 km[5] |
| 187±13 km[6] 205.495±1.881[1] 189 km[7] | |
| Flattening | 0.35[a] |
| Mass | (6.1±0.9)×1018 kg[6] ≈ 6.8×1018 kg[b] |
Mean density | 1.78±0.45 g/cm3[6] ≈ 1.95 g/cm³[5] |
| 5.988 hr[1] | |
| 0.052 (calculated)[6] 0.059±0.007[1] | |
| C[1] | |
| 7.61[1] | |
41 Daphne is a large asteroid from the asteroid belt.[1] It is a dark-surfaced body 174 km in diameter is probably composed of primitive carbonaceous chondrites. The spectra of the asteroid displays evidence of aqueous alteration.[8] It was discovered by H. Goldschmidt on May 22, 1856, and named after Daphne, the nymph in Greek mythology who was turned into a laurel tree. Incorrect orbital calculations initially resulted in 56 Melete being mistaken for a second sighting of Daphne. Daphne was not sighted again until August 31, 1862.[9]
The orbit of 41 Daphne places it in a 9:22 mean motion resonance with the planet Mars. The computed Lyapunov time for this asteroid is 14,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because of gravitational perturbations of the planets.[10]
In 1999, Daphne occulted three stars, and on July 2, 1999, produced eleven chords indicating an ellipsoid of 213×160 km.[4] Daphnean lightcurves also suggest that the asteroid is irregular in shape. Daphne was observed by Arecibo radar in April 2008.[11][12] Based upon radar data, the near surface solid density of the asteroid is 2.4+0.7
−0.5 g cm−3.[13]
- ^ a b c d e f g h Cite error: The named reference
jpldatawas invoked but never defined (see the help page). - ^ "Daphne". Lexico UK English Dictionary. Oxford University Press. Archived from the original on 31 October 2020.
- ^ "Daphne". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ a b Cite error: The named reference
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Conrad2008was invoked but never defined (see the help page). - ^ a b c d e P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
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Fornasier1999was invoked but never defined (see the help page). - ^ Appletons' annual cyclopaedia and register of important events of the year: 1862. New York: D. Appleton & Company. 1863. p. 173.
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