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Latest revision Your text
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{{Planetbox begin

{{Short description|Hot Jupiter orbiting Kepler-419}}

| name = Kepler-419b

{{Infobox planet

| name = Kepler-419b

<!-- DISCOVERY -->

| discoverer = ''[[Kepler (spacecraft)|Kepler]]'' spacecraft

| discovered = 2012 (dubious)<br />12 June 2014 (confirmed)<ref name="Dawson" />

| discovery_method = [[Transit method]]<ref name="Dawson" />

<!-- DESIGNATIONS -->

<!-- ORBITAL -->

| apsis = astron

| semimajor = 0.37 (± 0.007)<ref name="Dawson" /> [[astronomical unit|AU]]

| eccentricity = 0.833 (± 0.013)<ref name="Dawson" />

| period = 69.7546 (± 0.0007)<ref name="Dawson" /> [[day|d]]

| inclination = {{val|88.95|0.14|0.17}}<ref name="Dawson"/>

| star = [[Kepler-419]] (KOI-1474)

<!-- PHYS CHARS -->

| mean_radius = 0.96 (± 0.12)<ref name="Dawson"/> {{Jupiter radius|link=y}}

| mass = 2.5 (± 0.3)<ref name="Dawson">{{Cite journal|arxiv=1405.5229 |title= Large eccentricity, low mutual inclination: The three-dimensional architecture of a hierarchical system of giant planets|journal= The Astrophysical Journal|volume= 791|issue= 2|pages= 89|last1= Dawson|first1= Rebekah I.|author2= John Asher Johnson|last3= Fabrycky|first3= Daniel C.|last4= Foreman-Mackey|first4= Daniel|last5= Murray-Clay|first5= Ruth A.|last6= Buchhave|first6= Lars A.|last7= Cargile|first7= Phillip A.|last8= Clubb|first8= Kelsey I.|last9= Fulton|first9= Benjamin J.|last10= Hebb|first10= Leslie|last11= Howard|first11= Andrew W.|last12= Huber|first12= Daniel|last13= Shporer|first13= Avi|last14= Valenti|first14= Jeff A.|year= 2014|doi= 10.1088/0004-637X/791/2/89|bibcode = 2014ApJ...791...89D |s2cid= 29630098}}</ref> {{Jupiter mass|link=y}}

| single_temperature = {{convert|505|K|C F}}

<!-- ATMOSPHERE -->

<!-- NOTES -->

}}

}}

{{Planetbox star

'''Kepler-419b''' (also known by its Kepler Object of Interest designation ''KOI-1474.01'') is a [[hot Jupiter]] [[exoplanet]] orbiting the star [[Kepler-419]], the outermost of two such planets discovered by [[NASA]]'s [[Kepler (spacecraft)|Kepler spacecraft]]. It is located about 3,400 [[light-year]]s (1040 [[parsec]]s from Earth in the constellation [[Cygnus (constellation)|Cygnus]].

| star = [[Kepler-419]] (KOI-1474)

| ra= {{RA|19|41|40.3}}

| dec= {{DEC|+51|11|05.15}}

| constell=[[Cygnus (constellation)|Cygnus]]

| app_mag = 13<ref name=kic>{{cite journal|bibcode= 2009yCat.5133....0K|title= VizieR Online Data Catalog: Kepler Input Catalog (Kepler Mission Team, 2009)|journal= VizieR On-line Data Catalog: V/133. Originally published in: 2009yCat.5133....0K|volume= 5133|author1= Kepler Mission Team|year= 2009}}</ref>

| dist_ly = 2544

| dist_pc = 780<ref name=dawson2012>{{cite journal|bibcode=2012ApJ...761..163D|arxiv=1206.5579|title=The Photoeccentric Effect and Proto-hot Jupiters. II. KOI-1474.01, a Candidate Eccentric Planet Perturbed by an Unseen Companion|journal=The Astrophysical Journal|volume=761|issue=2|pages=163|author1=Dawson|first1=Rebekah I.|last2=Johnson|first2=John Asher|last3=Morton|first3=Timothy D.|last4=Crepp|first4=Justin R.|last5=Fabrycky|first5=Daniel C.|last6=Murray-Clay|first6=Ruth A.|last7=Howard|first7=Andrew W.|year=2012|doi=10.1088/0004-637X/761/2/163}}</ref>

| class = F?V<ref name="Dawson"/>

| mass = 1.39 (± 0.08)<ref name="Dawson"/>

| radius = 1.75 (± 0.08)<ref name="Dawson"/>

| temperature = 6430 (± 79)<ref name="Dawson"/>

| metallicity = 0.176 (± 0.07)<ref name="Dawson"/>

| age = 2.8 (± 1.3)<ref name=EPE>{{cite web|url=http://exoplanet.eu/catalog/kepler-419_c/|title=Notes for planet Kepler-419 c|work=[[The Extrasolar Planets Encyclopedia]]|accessdate=August 8, 2016}}</ref>

}}

{{Planetbox character

| mass = 2.5 (± 0.3)<ref name="Dawson">{{Cite journal|last= |first= |author-link= |arxiv=1405.5229 |title= Large eccentricity, low mutual inclination: The three-dimensional architecture of a hierarchical system of giant planets|journal= The Astrophysical Journal|volume= 791|issue= 2|pages= 89|date= |last1= Dawson|first1= Rebekah I.|author2= John Asher Johnson|last3= Fabrycky|first3= Daniel C.|last4= Foreman-Mackey|first4= Daniel|last5= Murray-Clay|first5= Ruth A.|last6= Buchhave|first6= Lars A.|last7= Cargile|first7= Phillip A.|last8= Clubb|first8= Kelsey I.|last9= Fulton|first9= Benjamin J.|last10= Hebb|first10= Leslie|last11= Howard|first11= Andrew W.|last12= Huber|first12= Daniel|last13= Shporer|first13= Avi|last14= Valenti|first14= Jeff A.|year= 2014|doi= 10.1088/0004-637X/791/2/89}}</ref>

| radius = 0.96 (± 0.12)<ref name="Dawson"/>

| stellar_flux = 34.66

| temperature = {{convert|505|K|C F}}

}}

{{Planetbox orbit

| semimajor = 0.37 (± 0.007)<ref name="Dawson" />

| eccentricity = 0.833 (± 0.013)<ref name="Dawson" />

| period = 69.7546 (± 0.0007)<ref name="Dawson" />

| inclination = {{val|88.95|0.14|0.17}}<ref name="Dawson"/>

}}

{{Planetbox discovery

| discovery_date = 2012 (dubious)<br>12 June 2014 (confirmed)<ref name="Dawson" />

| discoverers = ''[[Kepler (spacecraft)|Kepler]]'' spacecraft

| discovery_method = [[Transit method]]<ref name="Dawson" />

| discovery_status = Published

}}

{{Planetbox catalog

| names = KOI-1474.01, KIC 12365184 b, WISE J194140.29+511105.1 b, 2MASS J19414029+5111051 b

}}

{{Planetbox reference

| star = Kepler-419

| planet = b

}}

{{Planetbox end}}



'''Kepler-419b''' (also known by its Kepler Object of Interest designation ''KOI-1474.01'') is a [[hot Jupiter]] [[exoplanet]] orbiting the star [[Kepler-419]], the outermost of two such planets discovered by [[NASA]]'s [[Kepler (spacecraft)|Kepler spacecraft]]. It is located about 2,544 [[light-year]]s (780 [[parsec]]s, or nearly {{val|2.4068|e=16}} [[km]]) from Earth in the constellation [[Cygnus (constellation)|Cygnus]].<ref name="Dawson"/> The exoplanet was found by using the [[transit method]], in which the dimming effect that a planet causes as it crosses in front of its star is measured.

==Characteristics==


== Characteristics ==



===Mass, radius and temperature===

===Mass, radius and temperature===

Kepler-419b is a [[hot Jupiter]], an exoplanet that has a radius and mass near that of the planet [[Jupiter]], but with a much higher temperature. It has a temperature of {{convert|505|K|C F}}.<ref name="PHL">[http://www.hpcf.upr.edu/~abel/phl/hec_plots/hec_orbit/hec_orbit_Kepler-419_b.png Kepler 419] hpcf.upr.edu</ref> It has a mass of 2.5 {{Jupiter mass}} and a radius of 0.96 {{Jupiter radius}}.

Kepler-419b is a [[hot Jupiter]], an exoplanet that has a radius and mass near that of the planet [[Jupiter]], but with an extremely high temperature. It has a temperature of {{convert|505|K|C F}}.<ref name="PHL">http://www.hpcf.upr.edu/~abel/phl/hec_plots/hec_orbit/hec_orbit_Kepler-419_b.png</ref> It has a mass of 2.5 {{Jupiter mass}} and a radius of 0.96 {{Jupiter radius}}.



===Host star===

===Host star===

The planet orbits an ([[Stellar classification#Class F|F-type]]) [[star]] named [[Kepler-419]]. The star has a mass of 1.39 {{Solar mass}} and a radius 1.75 {{Solar radius}}. It has a surface temperatures of 6430 [[Kelvin|K]] and is 2.8 billion years old. In comparison, the Sun is about 4.6 billion years old<ref>{{cite web |url=http://www.universetoday.com/18237/how-old-is-the-sun/ |title=How Old is the Sun? |author=Fraser Cain |date=16 September 2008 |publisher=Universe Today |access-date=19 February 2011}}</ref> and has a surface temperature of 5778 K.<ref>{{cite web |url=http://www.universetoday.com/18092/temperature-of-the-sun/ |title=Temperature of the Sun |author=Fraser Cain |date=September 15, 2008 |publisher=Universe Today |access-date=19 February 2011}}</ref>

The planet orbits an ([[Stellar classification#Class F|F-type]]) [[star]] named [[Kepler-419]]. The star has a mass of 1.39 {{Solar mass}} and a radius 1.75 {{Solar radius}}. It has a surface temperatures of 6430 [[Kelvin|K]] and is 2.8 billion years old. In comparison, the Sun is about 4.6 billion years old<ref>{{cite web |url=http://www.universetoday.com/18237/how-old-is-the-sun/ |title=How Old is the Sun? |author=Fraser Cain |date=16 September 2008 |work= |publisher=Universe Today |accessdate=19 February 2011}}</ref> and has a surface temperature of 5778 K.<ref>{{cite web |url=http://www.universetoday.com/18092/temperature-of-the-sun/ |title=Temperature of the Sun |author=Fraser Cain |date=September 15, 2008 |work= |publisher=Universe Today |accessdate=19 February 2011}}</ref>



The star's [[apparent magnitude]], or how bright it appears from Earth's perspective, is 13. It is too dim to be seen with the naked eye.

The star's [[apparent magnitude]], or how bright it appears from Earth's perspective, is 13. It is too dim to be seen with the naked eye.



===Orbit===

=== Orbit ===



Kepler-419c orbits its host star with 270% of the Sun's luminosity (2.7 {{solar luminosity}}) about every 67 days at a distance of 0.37 [[astronomical unit|AU]] (close to the orbital distance of Mercury from the Sun, which is 0.38 AU). It has a highly eccentric orbit, with an eccentricity of 0.833.

Kepler-419c orbits its host star with 270% of the Sun's luminosity (2.7 {{solar luminosity}}) about every 67 days at a distance of 0.37 [[astronomical unit|AU]] (close to the orbital distance of Mercury from the Sun, which is 0.38 AU). It has a highly eccentric orbit, with an eccentricity of 0.833.



==Discovery==

==Discovery==

In 2009, [[NASA]]'s [[Kepler (spacecraft)|Kepler]] spacecraft was completing observing stars on its [[photometer]], the instrument it uses to detect [[transit method|transit]] events, in which a planet crosses in front of and dims its host star for a brief and roughly regular period of time. In this last test, Kepler observed {{val|50,000}} stars in the [[Kepler Input Catalog]], including Kepler-419, the preliminary light curves were sent to the Kepler science team for analysis, who chose obvious planetary companions from the bunch for follow-up at observatories. Observations for the potential exoplanet candidates took place between 13 May 2009 and 17 March 2012. After observing the respective transits, the first planet, Kepler-419b, was announced.<ref name="Dawson"/>

In 2009, [[NASA]]'s [[Kepler (spacecraft)|Kepler]] spacecraft was completing observing stars on its [[photometer]], the instrument it uses to detect [[transit method|transit]] events, in which a planet crosses in front of and dims its host star for a brief and roughly regular period of time. In this last test, Kepler observed {{val|50,000}} stars in the [[Kepler Input Catalog]], including Kepler-419, the preliminary light curves were sent to the Kepler science team for analysis, who chose obvious planetary companions from the bunch for follow-up at observatories. Observations for the potential exoplanet candidates took place between 13 May 2009 and 17 March 2012. After observing the respective transits, the first planet, Kepler-419b, was announced.



==References==

==References==

{{reflist|refs=

{{reflist}}


}}



==External links==

==External links==

* [https://web.archive.org/web/20131105082102/http://www.nasa.gov/mission_pages/kepler/main/index.html NASA – Kepler Mission].

* [http://www.nasa.gov/mission_pages/kepler/main/index.html NASA – Kepler Mission].

* [https://web.archive.org/web/20100527104316/http://kepler.nasa.gov/Mission/discoveries/ NASA – Kepler Discoveries – Summary Table].

* [http://kepler.nasa.gov/Mission/discoveries/ NASA – Kepler Discoveries – Summary Table].

* [http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-419+b&type=CONFIRMED_PLANET NASA – Kepler-419b] at [[NASA Exoplanet Archive|The NASA Exoplanet Archive]].

* [http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-419+b&type=CONFIRMED_PLANET NASA – Kepler-419b] at [[NASA Exoplanet Archive|The NASA Exoplanet Archive]].

* [http://exoplanets.org/detail/Kepler-419_b NASA – Kepler-419b] at [[Exoplanet Data Explorer|The Exoplanet Data Explorer]].

* [http://exoplanets.org/detail/Kepler-419_b NASA – Kepler-419b] at [[Exoplanet Data Explorer|The Exoplanet Data Explorer]].

* [https://exoplanet.eu/catalog/kepler_419_b--1197/ NASA – Kepler-419b] at [[Extrasolar Planets Encyclopaedia|The Extrasolar Planets Encyclopaedia]].

* [http://exoplanet.eu/catalog/kepler-419_b/ NASA – Kepler-419b] at [[Extrasolar Planets Encyclopaedia|The Extrasolar Planets Encyclopaedia]].



{{Exoplanets}}

{{Exoplanets}}

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{{Extraterrestrial life}}

{{Extraterrestrial life}}

{{2014 in space}}

{{2014 in space}}

{{Portal bar|Astronomy|Biology}}

{{portal bar|Astrobiology|Astronomy}}

{{Sky|19|41|40.3|+|51|11|05.15}}

{{Sky|19|41|40.3|+|51|11|05.15}}



[[Category:Exoplanets discovered by the Kepler space telescope]]

[[Category:Exoplanets discovered by Kepler (spacecraft)]]

[[Category:Giant planets]]

[[Category:Giant planets]]

[[Category:Exoplanets discovered in 2014]]

[[Category:Exoplanets discovered in 2014]]

[[Category:Transiting exoplanets]]

[[Category:Transiting exoplanets]]

[[Category:Cygnus (constellation)]]

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