2608 Seneca

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2608 Seneca
Discovery [1]
Discovered by H.-E. Schuster
Discovery site La Silla Obs.
Discovery date17 February 1978
Designations
(2608) Seneca
Pronunciation /ˈsɛnɪkə/ SEN-ik-ə [2]
Named after
Seneca the Younger
(Roman philosopher) [3]
1978 DA
NEO  · Amor [1] [4]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 1
Observation arc 38.92 yr (14,217 days)
Aphelion 3.9532 AU
Perihelion 1.0777 AU
2.5154 AU
Eccentricity 0.5716
3.99 yr (1,457 days)
353.12°
0° 14m 49.56s / day
Inclination 14.682°
167.37°
37.350°
Earth  MOID 0.1321 AU ·51.5 LD
Physical characteristics
Dimensions 0.9 km [1] [5] [6]
1.0±0.3 [6]
8 h [6]
0.15±0.03 [6]
0.20 (derived) [5]
0.21 [1]
Tholen = S [1]  · S [5]
B–V = 0.826 [1]
U–B = 0.454 [1]
17.52 [1]  ·17.59 [5] [7]  ·17.73 [6]

    2608 Seneca, provisional designation 1978 DA, is a stony asteroid and sub-kilometer near-Earth object of the Amor group, approximately 0.9 kilometers in diameter. It was discovered on 17 February 1978, by German astronomer Hans-Emil Schuster at ESO's La Silla Observatory in northern Chile, and named after Roman philosopher Seneca. [3] [4]

    Contents

    Orbit

    Seneca orbits the Sun at a distance of 1.1–4.0  AU once every 3 years and 12 months (1,457 days). Its orbit has an eccentricity of 0.57 and an inclination of 15° with respect to the ecliptic. [1]

    The body's observation arc begins with its official discovery observation in 1978, as no precoveries were taken, and no prior identifications were made. [4]

    Close approaches

    Seneca has an Earth minimum orbital intersection distance of 0.1321 AU (19,800,000 km), which corresponds to 51.5 lunar distances. [1] On 22 March 2062, it will pass 0.254 AU (38,000,000 km) from the Earth. [8]

    Physical characteristics

    In the Tholen taxonomy, Seneca is a stony S-type asteroid. [1]

    Photometry

    In March 1978, a photometric observations taken by Degewij and Lebofsky at the Lunar and Planetary Laboratory, Arizona, using a 154-cm reflector, gave a rotational lightcurve with a rotation period of 8 hours and a brightness amplitude of 0.4 (0.5) magnitude ( U=2 ). [6]

    Radiometry

    In addition, radiometric observations by L. and M. Lebofsky with the 71-cm reflector gave a mean-diameter of 1.0±0.3 kilometers and albedo of 0.15±0.03. [6]

    Diameter and albedo

    The Minor Planet Center classifies Seneca as an object larger than 1 kilometer ("1+ KM Near-Earth Object"), [4] while Collaborative Asteroid Lightcurve Link derives an albedo of 0.20 and a diameter of 0.9 kilometers based on an absolute magnitude of 17.59. [5] In 1994, astronomer Tom Gehrels published a diameter of 0.9 kilometers with an albedo of 0.21 in his Hazards Due to Comets and Asteroids. [1]

    Naming

    This minor planet was named after Roman philosopher and statesman Lucius Annaeus Seneca (c. 4 BC – AD 65), also known as "Seneca the Younger" or simply "Seneca". [3] The approved naming citation was published by the Minor Planet Center on 8 April 1982 ( M.P.C. 6835). [9] The lunar crater Seneca was also named in his honor. [3]

    References

    1. 1 2 3 4 5 6 7 8 9 10 11 12 13 "JPL Small-Body Database Browser: 2608 Seneca (1978 DA)" (2017-01-20 last obs.). Jet Propulsion Laboratory . Retrieved 3 July 2017.
    2. "Seneca" . Oxford English Dictionary (Online ed.). Oxford University Press.(Subscription or participating institution membership required.)
    3. 1 2 3 4 Schmadel, Lutz D. (2007). "(2608) Seneca". Dictionary of Minor Planet Names – (2608) Seneca. Springer Berlin Heidelberg. p. 213. doi:10.1007/978-3-540-29925-7_2609. ISBN   978-3-540-00238-3.
    4. 1 2 3 4 "2608 Seneca (1978 DA)". Minor Planet Center. Retrieved 26 March 2017.
    5. 1 2 3 4 5 "LCDB Data for (2608) Seneca". Asteroid Lightcurve Database (LCDB). Retrieved 26 March 2017.
    6. 1 2 3 4 5 6 7 Degewij, J.; Lebofsky, L.; Lebofsky, M. (March 1978). "1978 CA and 1978 DA". IAU Circ. 3193 (3193): 1. Bibcode:1978IAUC.3193....1D . Retrieved 26 March 2017.
    7. Schuster, H. E.; Surdej, A.; Surdej, J. (September 1979). "Photoelectric observations of two unusual asteroids - 1978 CA and 1978 DA". Astronomy and Astrophysics Supplement Series. 37: 483–486. Bibcode:1979A&AS...37..483S . Retrieved 26 March 2017.
    8. "JPL Close-Approach Data: 2608 Seneca (1978 DA)" (2010-08-19 last obs). Retrieved 15 April 2016.
    9. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 26 March 2017.