41 Daphne

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41 Daphne
File:41 Daphne VLT (2021), deconvolved.pdf
Discovery[1]
Discovered byH. Goldschmidt
Discovery dateMay 22, 1856
Designations
(41) Daphne
Pronunciation/ˈdæfni/[2]
Named after
Daphne
1949 TG
Main belt
AdjectivesDaphnean /ˈdæfniən/[3]
Orbital characteristics[1]
Epoch 31 December 2006 (JD 2454100.5)
Aphelion3.517 AU (526.144 million km)
Perihelion2.014 AU (301.220 million km)
2.765 AU (413.682 million km)
Eccentricity0.272
4.60 a (1,679.618 d)
247.500°
Inclination15.765°
178.159°
46.239°
Known satellitesPeneius /pɛˈnəs/
(S/2008 (41) 1)
Physical characteristics
Dimensions213×160 km[4]
239x183x153 km[5]
187±13 km[6]
205.495±1.881[1]
189 km[7]
Flattening0.35[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]

Satellite

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Peneius
File:41Daphne-Keck.jpg
Daphne and Peneius as seen by the W.M. Keck II telescope in 2008
Designations
(41) Daphne I
Pronunciation/pɛˈnəs/
S/2008 (41) 1
AdjectivesPeneian /pɛˈnən/
Orbital characteristics
Inclination°

41 Daphne has at least one satellite, named Peneius (provisionally S/2008 (41) 1).[14][15] It was identified on March 28, 2008, and has a projected separation of 443 km, an orbital period of approximately 1.1 days,[5] and an estimated diameter of less than 2 km. If these preliminary observations hold up, this binary system has the most extreme size ratio known.[16] In Greek myth, Pēneios is the god of the river of that name, and father of Daphne.

Notes

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  1. ^ Flattening derived from the maximum aspect ratio (c/a): f=1ca, where (c/a) = 0.65±0.08.[6]
  2. ^ Using the formula for volume of an ellipsoid (m = v × d), 239 × 183 × 153 km times a density of 1.95 g/cm3 yields a mass of 6.8×1018 kg

References

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  1. ^ a b c d e f g h Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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  3. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). (Subscription or participating institution membership required.)
  4. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). (1999-Jul-02 Chords)
  5. ^ a b c Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  6. ^ 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
  7. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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  16. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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vec:Lista de asteroidi#41 Dafne