HD 7924 - Revision history

AluminiumWithAnI: fixed citation error

2024-09-22T09:22:54Z

fixed citation error

← Previous revision		Revision as of 09:22, 22 September 2024
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	\| doi=10.1134/S1063773712050015 \| s2cid=119257644 }}</ref>		\| doi=10.1134/S1063773712050015 \| s2cid=119257644 }}</ref>

	<ref name=Høg2000>{{Cite ~~book~~		<ref name=Høg2000>{{Cite journal
	\| display-authors=1 \| last1=Høg \| first1=E.		\| display-authors=1 \| last1=Høg \| first1=E.
	\| last2=Fabricius \| first2=C. \| last3=Makarov \| first3=V. V.		\| last2=Fabricius \| first2=C. \| last3=Makarov \| first3=V. V.

Citation bot: Added doi-access. | Use this bot. Report bugs. | Suggested by Headbomb | Linked from Wikipedia:WikiProject_Academic_Journals/Journals_cited_by_Wikipedia/Sandbox | #UCB_webform_linked 491/559

2024-08-23T03:52:22Z

Added doi-access. | Use this bot. Report bugs. | Suggested by Headbomb | Linked from Wikipedia:WikiProject_Academic_Journals/Journals_cited_by_Wikipedia/Sandbox | #UCB_webform_linked 491/559

← Previous revision		Revision as of 03:52, 23 August 2024
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	\| volume=438 \| issue=3 \| pages=2413–2425 \| year=2014		\| volume=438 \| issue=3 \| pages=2413–2425 \| year=2014
	\| arxiv=1312.1792 \| bibcode=2014MNRAS.438.2413V		\| arxiv=1312.1792 \| bibcode=2014MNRAS.438.2413V
	\| doi=10.1093/mnras/stt2360 }}</ref>		\| doi=10.1093/mnras/stt2360 \| doi-access=free }}</ref>

	<ref name=berkeley>{{cite web		<ref name=berkeley>{{cite web

Citation bot: Add: doi-access. | Use this bot. Report bugs. | #UCB_CommandLine

2023-08-24T21:04:42Z

Add: doi-access. | Use this bot. Report bugs. | #UCB_CommandLine

← Previous revision		Revision as of 21:04, 24 August 2023
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	\| volume=153 \| issue=1 \| id=21 \| pages=19 \| date=January 2017		\| volume=153 \| issue=1 \| id=21 \| pages=19 \| date=January 2017
	\| bibcode=2017AJ....153...21L \| arxiv=1611.02897		\| bibcode=2017AJ....153...21L \| arxiv=1611.02897
	\| doi=10.3847/1538-3881/153/1/21 \| s2cid=119511744 \| postscript=. }}</ref>		\| doi=10.3847/1538-3881/153/1/21 \| s2cid=119511744 \| postscript=. \| doi-access=free }}</ref>

	<ref name=BailerJones2018>{{cite journal		<ref name=BailerJones2018>{{cite journal
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	\| volume=799 \| issue=1 \| at=105 \| year=2016		\| volume=799 \| issue=1 \| at=105 \| year=2016
	\| arxiv=1411.5374 \| bibcode=2016ApJ...830..105K		\| arxiv=1411.5374 \| bibcode=2016ApJ...830..105K
	\| doi=10.3847/0004-637X/830/2/105 \| s2cid=118542104 }}</ref>		\| doi=10.3847/0004-637X/830/2/105 \| s2cid=118542104 \| doi-access=free }}</ref>

	}}		}}

The Space Enthusiast at 09:43, 14 November 2022

2022-11-14T09:43:16Z

← Previous revision		Revision as of 09:43, 14 November 2022
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	{{short description\|~~Orange-hued hydrogen-burning~~ in the constellation Cassiopeia}}		{{short description\|Star in the constellation Cassiopeia}}
	{{Starbox begin}}		{{Starbox begin}}
	{{Starbox image		{{Starbox image

The Space Enthusiast at 06:08, 2 November 2022

2022-11-02T06:08:01Z

← Previous revision		Revision as of 06:08, 2 November 2022
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	{{short description\|K-~~type~~ ~~main sequence star~~ in the constellation Cassiopeia}}		{{short description\|Orange-hued hydrogen-burning in the constellation Cassiopeia}}
	{{Starbox begin}}		{{Starbox begin}}
	{{Starbox image		{{Starbox image

The Space Enthusiast at 03:48, 6 July 2022

2022-07-06T03:48:35Z

← Previous revision		Revision as of 03:48, 6 July 2022
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	{{short description\|~~Star~~ in the constellation Cassiopeia}}		{{short description\|K-type main sequence star in the constellation Cassiopeia}}
	{{Starbox begin}}		{{Starbox begin}}
	{{Starbox image		{{Starbox image
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	This is a [[K-type main-sequence star]] with a [[stellar classification]] of K0.5V.<ref name=vonBraun2014/> Low-level [[magnetic activity\|chromospheric activity]] has been detected, with the star showing spots and an activity cycle.<ref name="Fulton2015"/> The star is about three<ref name="Bonfanti2015"/> billion years old and is spinning with a [[projected rotational velocity]] of just 0.9 km/s.<ref name=Earle2017/> It has 81% of the [[mass of the Sun]] and 74% of the [[Sun's radius]]. The [[metallicity\|metal]] content is about seven-tenths as much as the Sun. It is radiating 36.4% of the [[luminosity of the Sun]] from its [[photosphere]] at an [[effective temperature]] of 5,216 K.<ref name="Bonfanti2015"/>		This is a [[K-type main-sequence star]] with a [[stellar classification]] of K0.5V.<ref name=vonBraun2014/> Low-level [[magnetic activity\|chromospheric activity]] has been detected, with the star showing spots and an activity cycle.<ref name="Fulton2015"/> The star is about three<ref name="Bonfanti2015"/> billion years old and is spinning with a [[projected rotational velocity]] of just 0.9 km/s.<ref name=Earle2017/> It has 81% of the [[mass of the Sun]] and 74% of the [[Sun's radius]]. The [[metallicity\|metal]] content is about seven-tenths as much as the Sun. It is radiating 36.4% of the [[luminosity of the Sun]] from its [[photosphere]] at an [[effective temperature]] of 5,216 K.<ref name="Bonfanti2015"/>

	==Planetary system==		==Planetary system==
	In 2009, a [[super-Earth]] [[exoplanet]] was found in orbit around the star.<ref name="Howard2009"/> In 2015, two more planets were discovered, and the mass of the original planet was revised downwards slightly.<ref name=berkeley/><ref name="Fulton2015"/> It is possible that planets c and d are in the 8:5 [[Orbital resonance\|mean motion resonance]].<ref name="Kane2016"/> All of the planets lie inside the star's [[habitable zone]].<ref name="Fulton2015"/>		In 2009, a [[super-Earth]] [[exoplanet]] was found in orbit around the star.<ref name="Howard2009"/> In 2015, two more planets were discovered, and the mass of the original planet was revised downwards slightly.<ref name=berkeley/><ref name="Fulton2015"/> It is possible that planets c and d are in the 8:5 [[Orbital resonance\|mean motion resonance]].<ref name="Kane2016"/> All of the planets lie inside the star's [[habitable zone]].<ref name="Fulton2015"/>

Trurle: sections and sorting

2021-09-20T21:48:14Z

sections and sorting

← Previous revision		Revision as of 21:48, 20 September 2021
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	This is a [[K-type main-sequence star]] with a [[stellar classification]] of K0.5V.<ref name=vonBraun2014/> Low-level [[magnetic activity\|chromospheric activity]] has been detected, with the star showing spots and an activity cycle.<ref name="Fulton2015"/> The star is about three<ref name="Bonfanti2015"/> billion years old and is spinning with a [[projected rotational velocity]] of just 0.9 km/s.<ref name=Earle2017/> It has 81% of the [[mass of the Sun]] and 74% of the [[Sun's radius]]. The [[metallicity\|metal]] content is about seven-tenths as much as the Sun. It is radiating 36.4% of the [[luminosity of the Sun]] from its [[photosphere]] at an [[effective temperature]] of 5,216 K.<ref name="Bonfanti2015"/>		This is a [[K-type main-sequence star]] with a [[stellar classification]] of K0.5V.<ref name=vonBraun2014/> Low-level [[magnetic activity\|chromospheric activity]] has been detected, with the star showing spots and an activity cycle.<ref name="Fulton2015"/> The star is about three<ref name="Bonfanti2015"/> billion years old and is spinning with a [[projected rotational velocity]] of just 0.9 km/s.<ref name=Earle2017/> It has 81% of the [[mass of the Sun]] and 74% of the [[Sun's radius]]. The [[metallicity\|metal]] content is about seven-tenths as much as the Sun. It is radiating 36.4% of the [[luminosity of the Sun]] from its [[photosphere]] at an [[effective temperature]] of 5,216 K.<ref name="Bonfanti2015"/>
			==Planetary system==

	In 2009, a [[super-Earth]] [[exoplanet]] was found in orbit around the star.<ref name="Howard2009"/> In 2015, two more planets were discovered, and the mass of the original planet was revised downwards slightly.<ref name=berkeley/><ref name="Fulton2015"/> It is possible that planets c and d are in the 8:5 [[Orbital resonance\|mean motion resonance]].<ref name="Kane2016"/> All of the planets lie inside the star's [[habitable zone]].<ref name="Fulton2015"/>		In 2009, a [[super-Earth]] [[exoplanet]] was found in orbit around the star.<ref name="Howard2009"/> In 2015, two more planets were discovered, and the mass of the original planet was revised downwards slightly.<ref name=berkeley/><ref name="Fulton2015"/> It is possible that planets c and d are in the 8:5 [[Orbital resonance\|mean motion resonance]].<ref name="Kane2016"/> All of the planets lie inside the star's [[habitable zone]].<ref name="Fulton2015"/>

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	[[Category:Henry Draper Catalogue objects\|007924]]		[[Category:Henry Draper Catalogue objects\|007924]]
	[[Category:Hipparcos objects\|006379]]		[[Category:Hipparcos objects\|006379]]
			[[Category:2MASS objects\|J01215911+7642372]]

Citation bot: Alter: template type. Add: s2cid. | Use this bot. Report bugs. | Suggested by Abductive | Category:Durchmusterung objects | #UCB_Category 2059/3725

2021-06-26T17:59:11Z

Alter: template type. Add: s2cid. | Use this bot. Report bugs. | Suggested by Abductive | Category:Durchmusterung objects | #UCB_Category 2059/3725

← Previous revision		Revision as of 17:59, 26 June 2021
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	\| volume=153 \| issue=1 \| id=21 \| pages=19 \| date=January 2017		\| volume=153 \| issue=1 \| id=21 \| pages=19 \| date=January 2017
	\| bibcode=2017AJ....153...21L \| arxiv=1611.02897		\| bibcode=2017AJ....153...21L \| arxiv=1611.02897
	\| doi=10.3847/1538-3881/153/1/21 \| postscript=. }}</ref>		\| doi=10.3847/1538-3881/153/1/21 \| s2cid=119511744 \| postscript=. }}</ref>

	<ref name=BailerJones2018>{{cite journal		<ref name=BailerJones2018>{{cite journal
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	\| volume=616 \| pages=A37 \| date=2018		\| volume=616 \| pages=A37 \| date=2018
	\| arxiv=1805.07581 \| bibcode=2018A&A...616A..37B		\| arxiv=1805.07581 \| bibcode=2018A&A...616A..37B
	\| doi=10.1051/0004-6361/201833456 }}</ref>		\| doi=10.1051/0004-6361/201833456 \| s2cid=56269929 }}</ref>

	<ref name=Anderson2012>{{cite journal		<ref name=Anderson2012>{{cite journal
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	\| volume=38 \| issue=5 \| pages=331 \| year=2012		\| volume=38 \| issue=5 \| pages=331 \| year=2012
	\| bibcode=2012AstL...38..331A \| arxiv=1108.4971		\| bibcode=2012AstL...38..331A \| arxiv=1108.4971
	\| doi=10.1134/S1063773712050015 }}</ref>		\| doi=10.1134/S1063773712050015 \| s2cid=119257644 }}</ref>

	<ref name=Høg2000>{{Cite book		<ref name=Høg2000>{{Cite book
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	\| bibcode=2000A&A...355L..27H }}</ref>		\| bibcode=2000A&A...355L..27H }}</ref>

	<ref name=Cutri2003>{{cite ~~journal~~		<ref name=Cutri2003>{{cite book
	\| last1=Cutri \| first1=R. M. \| last2=Skrutskie \| first2=M. F.		\| last1=Cutri \| first1=R. M. \| last2=Skrutskie \| first2=M. F.
	\| last3=van Dyk \| first3=S. \| last4=Beichman \| first4=C. A.		\| last3=van Dyk \| first3=S. \| last4=Beichman \| first4=C. A.
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	\| volume=575 \| at=A18 \| year=2015		\| volume=575 \| at=A18 \| year=2015
	\| arxiv=1411.4302 \| bibcode=2015A&A...575A..18B		\| arxiv=1411.4302 \| bibcode=2015A&A...575A..18B
	\| doi=10.1051/0004-6361/201424951 }}</ref>		\| doi=10.1051/0004-6361/201424951 \| s2cid=54555839
			}}</ref>

	<ref name="Fulton2015">{{cite journal		<ref name="Fulton2015">{{cite journal
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	\| volume=805 \| issue=2 \| pages=175 \| year=2015		\| volume=805 \| issue=2 \| pages=175 \| year=2015
	\| arxiv=1504.06629 \| bibcode=2015ApJ...805..175F		\| arxiv=1504.06629 \| bibcode=2015ApJ...805..175F
	\| doi=10.1088/0004-637X/805/2/175 }}</ref>		\| doi=10.1088/0004-637X/805/2/175 \| s2cid=7969255 }}</ref>

	<ref name="Howard2009">{{cite journal		<ref name="Howard2009">{{cite journal
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	\| volume=696 \| issue=1 \| pages=75–83 \| year=2009		\| volume=696 \| issue=1 \| pages=75–83 \| year=2009
	\| arxiv=0901.4394 \| bibcode=2009ApJ...696...75H		\| arxiv=0901.4394 \| bibcode=2009ApJ...696...75H
	\| doi=10.1088/0004-637X/696/1/75 }}</ref>		\| doi=10.1088/0004-637X/696/1/75 \| s2cid=1415310 }}</ref>

	<ref name="Kane2016">{{cite journal		<ref name="Kane2016">{{cite journal
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	\| volume=799 \| issue=1 \| at=105 \| year=2016		\| volume=799 \| issue=1 \| at=105 \| year=2016
	\| arxiv=1411.5374 \| bibcode=2016ApJ...830..105K		\| arxiv=1411.5374 \| bibcode=2016ApJ...830..105K
	\| doi=10.3847/0004-637X/830/2/105 }}</ref>		\| doi=10.3847/0004-637X/830/2/105 \| s2cid=118542104 }}</ref>

	}}		}}

Monkbot: Task 18b (cosmetic): eval 1 template: hyphenate params (1×);

2021-02-02T19:06:59Z

Task 18b (cosmetic): eval 1 template: hyphenate params (1×);

← Previous revision		Revision as of 19:06, 2 February 2021
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	{{Reflist\|refs=		{{Reflist\|refs=

	<ref name=SIMBAD>{{cite simbad \| title=HD 7924 \| ~~accessdate~~=2019-11-07}}</ref>		<ref name=SIMBAD>{{cite simbad \| title=HD 7924 \| access-date=2019-11-07}}</ref>

	<ref name="Gaia DR2">{{Cite Gaia DR2\|560130775546153344}}</ref>		<ref name="Gaia DR2">{{Cite Gaia DR2\|560130775546153344}}</ref>

Monkbot: Task 18 (cosmetic): eval 11 templates: hyphenate params (1×);

2021-01-29T03:14:06Z

Task 18 (cosmetic): eval 11 templates: hyphenate params (1×);

← Previous revision		Revision as of 03:14, 29 January 2021
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	\| title=Robotic telescope discovers three super-Earth planetary neighbors		\| title=Robotic telescope discovers three super-Earth planetary neighbors
	\| url=http://newscenter.berkeley.edu/2015/04/28/robotic-telescope-discovers-three-super-earth-planetary-neighbors/		\| url=http://newscenter.berkeley.edu/2015/04/28/robotic-telescope-discovers-three-super-earth-planetary-neighbors/
	\| ~~accessdate~~=2019-11-07 }}</ref>		\| access-date=2019-11-07 }}</ref>

	<ref name="Bonfanti2015">{{cite journal		<ref name="Bonfanti2015">{{cite journal

← Previous revision		Revision as of 21:04, 24 August 2023
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	\| volume=153 \| issue=1 \| id=21 \| pages=19 \| date=January 2017		\| volume=153 \| issue=1 \| id=21 \| pages=19 \| date=January 2017
	\| bibcode=2017AJ....153...21L \| arxiv=1611.02897		\| bibcode=2017AJ....153...21L \| arxiv=1611.02897
	\| doi=10.3847/1538-3881/153/1/21 \| s2cid=119511744 \| postscript=. }}</ref>		\| doi=10.3847/1538-3881/153/1/21 \| s2cid=119511744 \| postscript=. \| doi-access=free }}</ref>

	<ref name=BailerJones2018>{{cite journal		<ref name=BailerJones2018>{{cite journal
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	\| volume=799 \| issue=1 \| at=105 \| year=2016		\| volume=799 \| issue=1 \| at=105 \| year=2016
	\| arxiv=1411.5374 \| bibcode=2016ApJ...830..105K		\| arxiv=1411.5374 \| bibcode=2016ApJ...830..105K
	\| doi=10.3847/0004-637X/830/2/105 \| s2cid=118542104 }}</ref>		\| doi=10.3847/0004-637X/830/2/105 \| s2cid=118542104 \| doi-access=free }}</ref>

	}}		}}

← Previous revision		Revision as of 21:48, 20 September 2021
Line 61:		Line 61:

	This is a [[K-type main-sequence star]] with a [[stellar classification]] of K0.5V.<ref name=vonBraun2014/> Low-level [[magnetic activity\|chromospheric activity]] has been detected, with the star showing spots and an activity cycle.<ref name="Fulton2015"/> The star is about three<ref name="Bonfanti2015"/> billion years old and is spinning with a [[projected rotational velocity]] of just 0.9 km/s.<ref name=Earle2017/> It has 81% of the [[mass of the Sun]] and 74% of the [[Sun's radius]]. The [[metallicity\|metal]] content is about seven-tenths as much as the Sun. It is radiating 36.4% of the [[luminosity of the Sun]] from its [[photosphere]] at an [[effective temperature]] of 5,216 K.<ref name="Bonfanti2015"/>		This is a [[K-type main-sequence star]] with a [[stellar classification]] of K0.5V.<ref name=vonBraun2014/> Low-level [[magnetic activity\|chromospheric activity]] has been detected, with the star showing spots and an activity cycle.<ref name="Fulton2015"/> The star is about three<ref name="Bonfanti2015"/> billion years old and is spinning with a [[projected rotational velocity]] of just 0.9 km/s.<ref name=Earle2017/> It has 81% of the [[mass of the Sun]] and 74% of the [[Sun's radius]]. The [[metallicity\|metal]] content is about seven-tenths as much as the Sun. It is radiating 36.4% of the [[luminosity of the Sun]] from its [[photosphere]] at an [[effective temperature]] of 5,216 K.<ref name="Bonfanti2015"/>
			==Planetary system==

	In 2009, a [[super-Earth]] [[exoplanet]] was found in orbit around the star.<ref name="Howard2009"/> In 2015, two more planets were discovered, and the mass of the original planet was revised downwards slightly.<ref name=berkeley/><ref name="Fulton2015"/> It is possible that planets c and d are in the 8:5 [[Orbital resonance\|mean motion resonance]].<ref name="Kane2016"/> All of the planets lie inside the star's [[habitable zone]].<ref name="Fulton2015"/>		In 2009, a [[super-Earth]] [[exoplanet]] was found in orbit around the star.<ref name="Howard2009"/> In 2015, two more planets were discovered, and the mass of the original planet was revised downwards slightly.<ref name=berkeley/><ref name="Fulton2015"/> It is possible that planets c and d are in the 8:5 [[Orbital resonance\|mean motion resonance]].<ref name="Kane2016"/> All of the planets lie inside the star's [[habitable zone]].<ref name="Fulton2015"/>

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	[[Category:Henry Draper Catalogue objects\|007924]]		[[Category:Henry Draper Catalogue objects\|007924]]
	[[Category:Hipparcos objects\|006379]]		[[Category:Hipparcos objects\|006379]]
			[[Category:2MASS objects\|J01215911+7642372]]

← Previous revision		Revision as of 19:06, 2 February 2021
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	{{Reflist\|refs=		{{Reflist\|refs=

	<ref name=SIMBAD>{{cite simbad \| title=HD 7924 \| ~~accessdate~~=2019-11-07}}</ref>		<ref name=SIMBAD>{{cite simbad \| title=HD 7924 \| access-date=2019-11-07}}</ref>

	<ref name="Gaia DR2">{{Cite Gaia DR2\|560130775546153344}}</ref>		<ref name="Gaia DR2">{{Cite Gaia DR2\|560130775546153344}}</ref>