2608 Seneca
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]
| Discovery [1] | |
|---|---|
| Discovered by | H.-E. Schuster |
| Discovery site | La Silla Obs. |
| Discovery date | 17 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] | |
Orbit edit
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 edit
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 edit
In the Tholen taxonomy, Seneca is a stony S-type asteroid.[1]
Photometry edit
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 edit
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 edit
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 edit
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 edit
- ^ a b c d e f g h i j k l m "JPL Small-Body Database Browser: 2608 Seneca (1978 DA)" (2017-01-20 last obs.). Jet Propulsion Laboratory. Retrieved 3 July 2017.
- ^ "Seneca". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ a b c d 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.
- ^ a b c d "2608 Seneca (1978 DA)". Minor Planet Center. Retrieved 26 March 2017.
- ^ a b c d e "LCDB Data for (2608) Seneca". Asteroid Lightcurve Database (LCDB). Retrieved 26 March 2017.
- ^ a b c d e f g 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.
- ^ 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.
- ^ "JPL Close-Approach Data: 2608 Seneca (1978 DA)" (2010-08-19 last obs). Retrieved 15 April 2016.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 26 March 2017.
External links edit
- Hazards Due to Comets and Asteroids, Tom Gehrels (1994/5)
- Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- 2608 Seneca at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemerides · Observation prediction · Orbital info · MOID · Proper elements · Observational info · Close approaches · Physical info · Orbit animation
- 2608 Seneca at ESA–space situational awareness
- Ephemerides · Observations · Orbit · Physical properties · Summary
- 2608 Seneca at the JPL Small-Body Database