2002 GC32

| image = | caption = | discovery = yes | discovery_ref = | discoverer =M. W. Buie | discovery_site =807 | discovered = 2002/04/07 | designations = yes | mp_name = | alt_names = | mp_category = | orbit_ref = | epoch = | aphelion =45.625 | perihelion =41.321 | semimajor =43.473 | eccentricity =0.050 | period = | avg_speed = | inclination =2.7 | asc_node =67.2 | mean_anomaly =360.0 | arg_peri =137.4 | 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 =7.3

2002 GC32 adalah sebuah objek trans-Neptunus. Seperti objek trans-Neptunus pada umumnya, benda ini mengorbit Matahari dari jarak yang lebih jauh dari planet Neptunus.

Eksentrisitas orbit objek ini tercatat sebesar 0.050, sementara magnitudo mutlaknya adalah 7.3.

Rujukan

• Daftar Objek Transneptunus - The International Astronomical Union Minor Planet Center.
• Remo, John L. (2007). "Classifying Solid Planetary Bodies". AIP Conference Proceedings. 886: 284–302. Bibcode:2007AIPC..886..284R. doi:10.1063/1.2710063.