(508967) 2004 VC17: Perbedaan antara revisi

| minorplanet = yes

| width = 25em

| bgcolour =

| apsis =

| name = 2004 VC17

| symbol =

| image =

| caption =

| discovery = yes

| discovery_ref =

| discoverer =LINEAR

| discovery_site =704

| discovered = 2004/11/07

| designations = yes

| mp_name =

| alt_names =

| mp_category =

| orbit_ref =

| epoch =

| aphelion =3.434

| perihelion =0.360

| semimajor =1.897

| eccentricity =0.810

| period =

| avg_speed =

| inclination =20.4

| asc_node =229.6

| mean_anomaly =176.9

| arg_peri =64.8

| satellites =

| physical_characteristics = yes

| dimensions =

| mass =

| density =

| surface_grav =

| escape_velocity =

| sidereal_day =

| axial_tilt =

| pole_ecliptic_lat =

| pole_ecliptic_lon =

| albedo =

| temperatures=

| temp_name1 =

| mean_temp_1 =

| max_temp_1 =

| temp_name2 =

| max_temp_2 =

| spectral_type =

| abs_magnitude =18.4

Seperti asteroid pada umumnya, asteroid ini terbentuk dari [[nebula]] [[matahari]] primordial sebagai pecahan [[planetisimal]], sesuatu di nebula matahari muda yang tidak cukup besar untuk berubah menjadi planet.<ref>{{cite web | title=What Are Asteroids And Comets? | url=http://neo.jpl.nasa.gov/faq/#ast | work=Near Earth Object Program FAQ |publisher=[[NASA]] | accessdate=13 September 2010 | archiveurl=http://web.archive.org/web/20100909210213/http://neo.jpl.nasa.gov/faq/| archivedate=9 September 2010 | deadurl=no}}</ref>