2608 Seneca

{{Short description|Stony asteroid and sub-kilometer near-Earth object}}

{{Use dmy dates|date=October 2019}}

{{Infobox planet

| minorplanet = yes

| name = 2608 Seneca

| background = #FFC2E0

| image =

| image_size =

| caption =

| discovery_ref =

| discovered = 17 February 1978

| discoverer = H.-E. Schuster

| discovery_site = La Silla Obs.

| mpc_name = (2608) Seneca

| alt_names = 1978 DA

| pronounced = {{IPAc-en|ˈ|s|ɛ|n|ᵻ|k|ə}} {{respell|SEN|ik|ə}}{{OED|Seneca}}

| named_after = Seneca the Younger
{{small|(Roman philosopher)}}

| mp_category = NEO{{·}}Amor

| orbit_ref =

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 1

| observation_arc = 38.92 yr (14,217 days)

| aphelion = 3.9532 AU

| perihelion = 1.0777 AU

| semimajor = 2.5154 AU

| eccentricity = 0.5716

| period = 3.99 yr (1,457 days)

| mean_anomaly = 353.12°

| mean_motion = {{Deg2DMS|0.2471|sup=ms}} / day

| inclination = 14.682°

| asc_node = 167.37°

| arg_peri = 37.350°

| moid = 0.1321 AU{{·}}51.5 LD

| dimensions = 0.9 km
{{val|1.0|0.3}}

| rotation = {{val|8}} h

| albedo = {{val|0.15|0.03}}
0.20 {{small|(derived)}}
0.21

| spectral_type = Tholen = S{{·}}S
B–V = 0.826
U–B = 0.454

| abs_magnitude = 17.52{{·}}17.59{{·}}17.73

}}

2608 Seneca, provisional designation {{mp|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.

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.

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

= Close approaches =

Seneca has an Earth minimum orbital intersection distance of {{convert |0.1321 |AU |km |abbr=on |lk=off |sigfig=3}}, which corresponds to 51.5 lunar distances. On 22 March 2062, it will pass {{convert |0.254 |AU |km |abbr=on |lk=off |sigfig=3}} from the Earth.

Physical characteristics

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

= 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 ({{small|U=2}}).

= Radiometry =

In addition, radiometric observations by L. and M. Lebofsky with the 71-cm reflector gave a mean-diameter of {{val|1.0|0.3}} kilometers and albedo of {{val|0.15|0.03}}.

= Diameter and albedo =

The Minor Planet Center classifies Seneca as an object larger than 1 kilometer ("1+ KM Near-Earth Object"), 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. 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.

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". The approved naming citation was published by the Minor Planet Center on 8 April 1982 ({{small|M.P.C. 6835}}). The lunar crater Seneca was also named in his honor.

References

{{reflist|30em|refs=

{{cite web

|type = 2017-01-20 last obs.

|title = JPL Small-Body Database Browser: 2608 Seneca (1978 DA)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002608

|publisher = Jet Propulsion Laboratory

|accessdate = 3 July 2017}}

{{cite book

|title = Dictionary of Minor Planet Names – (2608) Seneca

|last = Schmadel | first = Lutz D.

|publisher = Springer Berlin Heidelberg

|page = 213

|date = 2007

|isbn = 978-3-540-00238-3

|doi = 10.1007/978-3-540-29925-7_2609 |chapter = (2608) Seneca }}

{{cite web

|title = 2608 Seneca (1978 DA)

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=2608

|accessdate = 26 March 2017}}

{{cite web

|title = MPC/MPO/MPS Archive

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html

|accessdate = 26 March 2017}}

{{cite web

|type = 2010-08-19 last obs

|title = JPL Close-Approach Data: 2608 Seneca (1978 DA)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Seneca;cad=1#cad

|accessdate = 15 April 2016}}

{{cite web

|title = LCDB Data for (2608) Seneca

|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2608%7CSeneca

|accessdate = 26 March 2017}}

{{Cite journal

|first1 = J. |last1 = Degewij

|first2 = L. |last2 = Lebofsky

|first3 = M. |last3 = Lebofsky

|date = March 1978

|title = 1978 CA and 1978 DA

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1978IAUC.3193....1D

|journal = IAU Circ.

|volume = 3193

|issue = 3193

|pages = 1

|bibcode = 1978IAUC.3193....1D

|access-date= 26 March 2017}}

{{Cite journal

|first1 = H. E. |last1 = Schuster

|first2 = A. |last2 = Surdej

|first3 = J. |last3 = Surdej

|date = September 1979

|title = Photoelectric observations of two unusual asteroids - 1978 CA and 1978 DA

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1979A&AS...37..483S

|journal = Astronomy and Astrophysics Supplement Series

|volume = 37

|pages = 483–486

|bibcode = 1979A&AS...37..483S

|access-date= 26 March 2017}}

}}