266P/Christensen

{{Infobox comet

| name=266P/Christensen

| image=

| discoverer=Eric J. Christensen

| discovery_date=October 27, 2006

| designations= 2006 U5

| epoch=2020-04-21.0

| semimajor=3.535 AU

| perihelion=2.335 AU

| aphelion=4.736 AU

| eccentricity=0.339

| period=6.65 a

| inclination= 3.426°

| last_p=2020-04-19
2013-08-31

| next_p=2026-Dec-07 (JPL Horizons last obs 2020-04-16)

}}

266P/Christensen is a periodic comet in the Solar System. It will next come to perihelion in December 2026. It has been suggested as the source of the 1977 "Wow! Signal".{{cite journal|last1=Paris|first1=Antonio|title=Hydrogen Clouds from Comets 266/P Christensen and P/2008 Y2 (Gibbs) are Candidates for the Source of the 1977 "WOW" Signal|journal=Washington Academy of Sciences|date=Winter 2015|url=http://planetary-science.org/wp-content/uploads/2016/01/Paris_Davies-H-I-Line-Signal.pdf|accessdate=7 June 2017}}

References

{{reflist

| refs =

{{cite web

|title=266P/Christensen Orbit

|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=266P

|publisher=Minor Planet Center

|accessdate=2017-06-08}}

{{cite web

|date=2014-02-27

|title=266P/Christensen (NK 2619)

|publisher=OAA Computing and Minor Planet Sections

|author=Syuichi Nakano

|author-link=Syuichi Nakano

|url=http://www.oaa.gr.jp/~oaacs/nk/nk2619.htm

|accessdate=2017-06-08}}

}}