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| ra = 10^h 56^m 38.6313170159^s | dec = −22 52 56.081842250° | appmag_v = 16.0^[1] }}

|}16h2i0i06a325l9743e0n3068t.spngM7sNgJ8ciq553p1198123671552

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This is the user sandbox of Kepler-1229b. A user sandbox is a subpage of the user's user page. It serves as a testing spot and page development space for the user and is not an encyclopedia article. Create or edit your own sandbox here.

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A a	B b	C c	Ç ç	D d	E e	Ə ə	F f
G g	H h	I i		J j	K k	L l	M m
N n	O o	Ɵ ɵ	P p	Q q	Ƣ ƣ	R r	S s
T t	U u	V v	X x	Y y	Z z	Ƶ ƶ

Alternate form[edit]

A letter composed of a short I with a hook can be found in the Yakut language. This may be an individual grapheme or simply a variant of Short I with tail.

| below = }}

K with oblique stroke[edit]

C with descender
C with descender
vfddfvdgtr
	File:Ooo
Usage
Writing system	Latin script
Type	alphabetic
Language of origin	Abkhaz language, Adyghe language, Kabardian language, Komi language, Udi language
Phonetic usage	[t͡sʼ], [t͡ɕ]
Unicode codepoint	unencoded
Alphabetical position	4th
History
Development	ج Γ γ 𐌂 C c vfddfvdgtr; ; ; ; ; ; ; ; ; ;
Time period	1920s-30s
Transliteration equivalents	Цӏ цӏ, Ч ч, Ҵ ҵ
Other
	This page contains phonetic transcriptions in the International Phonetic Alphabet (IPA). For an introductory guide on IPA symbols, see Help:IPA. For the distinction between [ ], / / and ⟨ ⟩, see IPA § Brackets and transcription delimiters.

2022 UQ₁
Discovery
Discovered by	ATLAS
Discovery site	El Sauce Obs.
Discovery date	18 October 2022
Designations
MPC designation	2022 UQ1
Minor planet category	NEO · Apollo (May 2020); Atira (Dec 2020)
Orbital characteristics
	Epoch 17 December 2020 (JD 2459200.5)
	Uncertainty parameter 2
Observation arc	167 days
Earliest precovery date	19 August 2020
Aphelion	0.988 AU
Perihelion	0.985 AU
Semi-major axis	0.986 AU
Eccentricity	0.00181
Orbital period (sidereal)	0.98 yr (357.9 d)
Mean anomaly	276.388°
Mean motion	1° 0m 21.877s / day
Inclination	0.1389°
Longitude of ascending node	216.656°
Argument of perihelion	311.989°
Earth MOID	0.01628 AU (May 2020); 0.00106 AU (Dec 2020)
Physical characteristics
Mean diameter	6–12 m (assumed)
Synodic rotation period	0.0026080±0.0000001 h; or 9.39 s
Apparent magnitude	22.4 (at discovery); 14.1 (1 Dec 2020)
Absolute magnitude (H)	27.66±0.34; 28.43

			Bilabial	Alveolar	Palatal	Velar	Uvular	Glottal
Nasal			m	n		ŋ
Plosive		voiceless	p	t		k	q	ʔ
Plosive		voiced	b	d		ɡ	ɢ
Fricative	central	voiceless		s	ç	(x)	(χ)	h
	central	voiced	β		ʝ	ɣ	ʁ
	lateral			ɮ
Affricate	lateral			t͡ɬ			qᵡ
Approximant	lateral			l
Flap				ɾ
Trill				r

β occurs as an allophone of b intervocalically.

	Front	Central	Back
Close	i	ɨ	u
Mid	ɛ^[a]	ə	ɔ^[a]
Open	a^[b]

List of pulsar planets[edit]

Confirmed planets[edit]

Pulsar	Planetary object	Mass	Semimajor axis (AU)	Orbital period	Discovered
PSR B1957+20	PSR B1957+20 b	22 M_J	−	0.38 d	1988
PSR B1620-26	PSR B1620-26 b	2.5 M_J	23	100.06849 y	2003
PSR B1257+12	PSR B1257+12 A	0.020 M_🜨	0.19	25.262±0.003 d	1994
	PSR B1257+12 B	4.3 M_🜨	0.36	66.5419±0.0001 d	1992
	PSR B1257+12 C	3.90 M_🜨	0.46	98.2114±0.0002 d	1992
PSR B0943+10	PSR B0943+10 b	2.8 M_J	1.8	730 d	2014
PSR B0943+10	PSR B0943+10 c	2.6 M_J	2.9	1460 d	2014
PSR B0329+54	PSR B0329+54 b	1.97 ± 0.19 M_🜨	10.26 ± 0.07	27.76 ± 0.03 y	2017
PSR J2322-2650	PSR J2322-2650 b	0.7949 M_J	0.0102	0.322963997 d	2017
PSR J2007+3120	PSR J2007+3120 b	0.0072 `M`_J	−	723±8 d	2022
PSR M13E	PSR M13E b	19.42^+3.0 _−0.0 M_J	−	0.11261745834±4e-11 d	2020
PSR J1719-1438	PSR J1719-1438 b	~1 M_J	0.004	2.176951032 h	2011
PSR J1544+4937	PSR J1544+4937 b	18 M_J	0.00537	0.1207729895±0.0000000001 d	2013
PSR J0636+5129	PSR J0636+5129 b	8 M_J	−	0.067 d	2016
PSR J2051-0827	PSR J2051-0827 b	28.3 M_J	−	0.099110266 d	1996
PSR J1807-2459 A	PSR J1807-2459 A b	9.4 M_J	−	0.07 d	2000

Candidate planets[edit]

Pulsar	Planetary object	Mass	Semimajor axis (AU)	Orbital period	Announced
PSR B1937+21	PSR B1937+21 b	~0.0001 `M`_E? ^{[citation needed]}	2.71	-	1999

Protoplanetary disks (fallback disks)[edit]

Pulsar	Protoplanetary disk	Discovered
4U 0142+61	debris disk	2006
1E 2259+586	candidate debris disk	2009^[8]

Disproven planets[edit]

Pulsar	Planet	Mass	Semimajor axis (AU)	Orbital period	Announced
Geminga	Geminga b	1.7 M_🜨	3.3	5.1 years	1997
PSR B1829-10	PSR 1829-10 A	10 M_🜨
PSR B1257+12	PSR B1257+12 D^[9]	0.0004 M_🜨
PSR B1828-10	PSR B1828-10 A	3 M_🜨	0.93	384.3649 days	1992
	PSR B1828-10 B	12 M_🜨	1.32	493.077375 days	1992
	PSR B1828-10 C	8 M_🜨	?	?	1992
PSR B0329+54	PSR B0329+54A	0.3 M_🜨
PSR B0329+54	PSR B0329+54B	2.2±0.002 M_🜨

^ Cite error: The named reference MNRAS4-022 was invoked but never defined (see the help page).
^ ^a ^b Cite error: The named reference MPEC-2020-S78 was invoked but never defined (see the help page).
^ ^a ^b ^c ^d Cite error: The named reference MPC-object was invoked but never defined (see the help page).
^ ^a ^b ^c Cite error: The named reference jpldata was invoked but never defined (see the help page).
^ Cite error: The named reference CNEOS was invoked but never defined (see the help page).
^ Peter Birtwhistle (Great Shefford Observatory). "Light curve".
^ Cite error: The named reference NEODy20201201 was invoked but never defined (see the help page).
^ Kaplan, David L.; Chakrabarty, Deepto; Wang, Zhongxiang; Wachter, Stefanie (July 2009). "A Mid-Infrared Counterpart to the Magnetar 1E 2259+586". Astrophysical Journal. 700 (1): 149–154. arXiv:0906.1604. Bibcode:2009ApJ...700..149K. doi:10.1088/0004-637X/700/1/149. ISSN 0004-637X. S2CID 9937378.
^ Wolszczan, Alex (January 2012). "Discovery of pulsar planets". New Astronomy Reviews. 56 (1). Elsevier: 2–8. Bibcode:2012NewAR..56....2W. doi:10.1016/j.newar.2011.06.002.

e[edit]

A a [a]	B b [b]	C c [t͡sʰ]	C' c' [t͡sʼ]	C° c°/Cw cw [t͡ɕʷ]	C'° c'°/C'w c'w [t͡ɕʷ’]	Č č [t͡ʃʰ]	Č' č' [t͡ʃʼ]
C̆ c̆ [t͡ʂʰ]	C̆' c̆' [t͡ʂʼ]	D d [d]	D° d°/Dw dw [dʷ]	Dz dz [d͡z]	Dz° dz°/Dzw dzw [d͡ʑʷ]	Dž dž [d͡ʐ]	Dzh dzh [d͡ʒ]
E e [e̞/aj/ja]	F f [f]	G g [ɡ]	Ǵ ǵ [ɡʲ]	G° g°/Gw gw [ɡʷ]	Ğ ğ [ʁ]	Ğ́ ğ́ [ʁʲ]	Ğ° ğ°/Ğw ğw [ʁʷ]
H h [χ]	H́ h́ [χʲ]	H° h°/Hw hw [χʷ]	ħ [ħ]	° ħ° [ħʷ]	I i [i]	J j [jə/əj]	K k [kʰ]
Ḱ ḱ [kʰʲ]	K° k°/Kw kw [kʷʰ]	K' k' [kʼ]	Ḱ' ḱ' [kʼʲ]	К'° k'°/K'w k'w [kʼʷ]	L l [l]	M m [m]	N n [n]
O o [o̞/aw/wa]	P p [pʰ]	P' p' [pʼ]	Q' q' [qʼ]	Q́' q́' [qʼʲ]	Q'° q'°/Q'w q'w [qʼʷ]	R r [r]	S s [s]
Š š [ʂ]	Š° š°/Šw šw [ʃʷ]	Sh sh [ʃ]	T t [tʰ]	T° t°/Tw tw [tʷʰ]	T' t' [tʼ]	T'° t'°/T'w t'w [tʼʷ]	U u [u]
W w [wə/əw]	Ɥ ɥ [ɥ/ɥˤ]	V v [v]	Y y [ə]	Z z [z]	Ž ž [ʐ]	Zh zh [ʒ]	Ž° ž°/Žw žw [ʒʷ]
(◌́) [ʲ]	(°/w) [ʷ]

additional latin[edit]

|-

! colspan="26" |

Additional Latin letters

2[edit]

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[[]]
[[]]
[[]]
[[]]
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[[]]
[]]
[[]]
[[]]
[[]]
[[]]
[[]]
[[]]
[[]]
[[]]
[[]]
[[]]
[[]]
ʕ
ǀ
ǁ
ǂ
ǃ
ʘ
ʻ
ˀ
ʼ
Ꞌ ꞌ
ᴬ
ᴮ
ꟲ
ᴰ
ᴱ
ꟳ
ᴳ
ᴴ
ᴵ
ᴶ
ᴷ
ᴸ
ᴹ
ᵃ
ᵉ
ᵋ
ʰ
ⁱ
ᶤ
ⁿ
ᵒ
ᵓ
ᵘ
ᶶ
ᵛ
ʷ
ʸ
ᶻ
ᶿ
Ꜣ ꜣ
Ꜥ ꜥ
3
7
⁷

etnos[edit]

Objets transneptuniens extrêmes

C with descender[edit]

C with descender is a letter of the Latin script, used in various latinized scripts for languages of the Soviet Union. Due to the shift of the alphabets of Soviet languages from Latin to Cyrillic, it fell out of use, and has not been encoded in Unicode. ^[1]^[2]

Usage[edit]

C with descender was used in the Abkhaz, Adyghe, Kabardian, Komi and Udi languages,^[1] representing the sound [t͡sʼ] in Adyghe, Abkhaz and Kabardian and [t͡ɕ] in Komi.

References[edit]

Cite error: There are <ref group=lower-alpha> tags or {{efn}} templates on this page, but the references will not show without a {{reflist|group=lower-alpha}} template or {{notelist}} template (see the help page).

^ ^a ^b "11360-soviet-latin.pdf" (PDF). 2011-10-18. Retrieved 5 April 2024.
^ "Rueter_2019-06-14_14232-n4502-form" (PDF). 2019-04-24. Retrieved 5 April 2024.

[MNRAS4-022-1] Cite error: The named reference MNRAS4-022 was invoked but never defined (see the help page).

[MPEC-2020-S78-2] Cite error: The named reference MPEC-2020-S78 was invoked but never defined (see the help page).

[MPC-object-3] Cite error: The named reference MPC-object was invoked but never defined (see the help page).

[jpldata-4] Cite error: The named reference jpldata was invoked but never defined (see the help page).

[CNEOS-5] Cite error: The named reference CNEOS was invoked but never defined (see the help page).

[Birtwhistle-6] Peter Birtwhistle (Great Shefford Observatory). "Light curve".

[NEODy20201201-7] Cite error: The named reference NEODy20201201 was invoked but never defined (see the help page).

[10] Kaplan, David L.; Chakrabarty, Deepto; Wang, Zhongxiang; Wachter, Stefanie (July 2009). "A Mid-Infrared Counterpart to the Magnetar 1E 2259+586". Astrophysical Journal. 700 (1): 149–154. arXiv:0906.1604. Bibcode:2009ApJ...700..149K. doi:10.1088/0004-637X/700/1/149. ISSN 0004-637X. S2CID 9937378.

[Wolszczan2012-11] Wolszczan, Alex (January 2012). "Discovery of pulsar planets". New Astronomy Reviews. 56 (1). Elsevier: 2–8. Bibcode:2012NewAR..56....2W. doi:10.1016/j.newar.2011.06.002.

[:0-12] "11360-soviet-latin.pdf" (PDF). 2011-10-18. Retrieved 5 April 2024.

[13] "Rueter_2019-06-14_14232-n4502-form" (PDF). 2019-04-24. Retrieved 5 April 2024.

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