class="wikitable sortable"
|+ Extremes |
| Record Title
!| Star
!| Date
!| Data
!width=100%| Notes
!| References |
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| {{nowrap|Least voluminous}} | EBLM J0555-57Ab | 2017 | r= {{convert|59000|km|mi|abbr=on}} | {{see|#List of least voluminous red dwarfs}} | [{{Cite journal |last=von Boetticher |first=Alexander |last2=Triaud |first2=Amaury H. M. J. |last3=Queloz |first3=Didier |last4=Gill |first4=Sam |last5=Lendl |first5=Monika |last6=Delrez |first6=Laetitia |last7=Anderson |first7=David R. |last8=Cameron |first8=Andrew Collier |last9=Faedi |first9=Francesca |last10=Gillon |first10=Michaël |last11=Chew |first11=Yilen Gómez Maqueo |last12=Hebb |first12=Leslie |last13=Hellier |first13=Coel |last14=Jehin |first14=Emmanuël |last15=Maxted |first15=Pierre F. L. |date=August 2017 |title=The EBLM project III. A Saturn-size low-mass star at the hydrogen-burning limit |url=http://arxiv.org/abs/1706.08781 |journal=Astronomy & Astrophysics |volume=604 |pages=L6 |doi=10.1051/0004-6361/201731107 |issn=0004-6361|arxiv=1706.08781 }}] |
| {{nowrap|Most voluminous}} | Sz74 | 2017 | {{val|3.13|0.72}} | {{see|#List of most voluminous red dwarfs}} | [{{citation
]| title=X-shooter spectroscopy of young stellar objects in Lupus. Accretion properties of class II and transitional objects
| last1=Alcalá | first1=J. M. | last2=Manara | first2=C. F.
| last3=Natta | first3=A. | last4=Frasca | first4=A.
| last5=Testi | first5=L. | last6=Nisini | first6=B.
| last7=Stelzer | first7=B. | last8=Williams | first8=J. P.
| last9=Antoniucci | first9=S. | last10=Biazzo | first10=K.
| last11=Covino | first11=E. | last12=Esposito | first12=M.
| last13=Getman | first13=F. | last14=Rigliaco | first14=E.
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=600 | id=A20 | pages=42 | postscript=.
| date=April 2017 | doi=10.1051/0004-6361/201629929
| arxiv=1612.07054 | bibcode=2017A&A...600A..20A | s2cid=119211262 }} |
| {{nowrap|Least massive}} | 2MASS J0523-1403 | 2015 | 67.54±12.79 {{Jupiter mass}} | {{see|#List of least massive red dwarfs}} | [{{Cite journal|last1=Filippazzo|first1=Joseph C.|last2=Rice|first2=Emily L.|last3=Faherty|first3=Jacqueline|author3-link=Jackie Faherty|last4=Cruz|first4=Kelle L.|last5=Gordon|first5=Mollie M. Van|last6=Looper|first6=Dagny L.|date=September 2015|journal=The Astrophysical Journal|volume=810|issue=2|page=158|doi=10.1088/0004-637X/810/2/158|issn=0004-637X|title=Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime|bibcode=2015ApJ...810..158F|arxiv=1508.01767|s2cid=89611607}}] |
| {{nowrap|Most massive}} | Kepler-80 | 2012 | 0.73 {{Solar mass}} | {{see|#List of most massive red dwarfs}} | [{{Cite web |last=Martin |first=Pierre-Yves |date=2023 |title=Planet Kepler-80 b |url=https://exoplanet.eu/catalog/kepler_80_b--1160/ |access-date=2023-11-01 |work=Extrasolar Planets Encyclopaedia |language=en}}] |
| {{nowrap|Least distant}} | {{nowrap|Proxima Centauri}} | 1917 | {{convert|4.2|ly|pc|abbr=on|lk=on}} | {{see|#List of nearest red dwarfs}}
This is also known as Alpha Centauri C and is a member of the α Cen trinary system. It is the nearest neighbouring star to the Sun. | |
| {{nowrap|Most distant}} | UDF 3561 | 2010 | 202,000 ly
(62,000 pc) | {{see|#List of furthest red dwarfs}} | [{{Cite journal|last1=Kilic|first1=Mukremin|last2=Gianninas|first2=Alexandros|last3=von Hippel|first3=Ted|title=Moving Objects in the Hubble Ultra Deep Field |date=2013-08-19|url=https://iopscience.iop.org/article/10.1088/0004-637X/774/1/88|journal=The Astrophysical Journal|language=en|volume=774|issue=1|page=88|doi=10.1088/0004-637x/774/1/88|arxiv=1307.5067 |bibcode=2013ApJ...774...88K |s2cid=118470451 |issn=0004-637X}}] |
| {{nowrap|Least luminous}} | 2MASS J0523-1403 | | | {{see|#List of least luminous red dwarfs}} | |
| {{nowrap|Most luminous}} | | | | {{see|#List of most luminous red dwarfs}} | |
| {{nowrap|Dimmest}} | UDF 2457 | | V= 25 | {{see|#List of dimmest red dwarfs}} | [{{Cite web |title=SKY-MAP.ORG - Interactive Sky Map |url=http://www.wikisky.org/?ra=3.5441034&de=-27.80278&zoom=15&show_grid=1&show_constellation_lines=1&show_constellation_boundaries=1&show_const_names=1&show_galaxies=1&show_box=1&box_ra=3.5441034&box_de=-27.80278&box_width=50&box_height=50&img_source=IMG_all |access-date=2023-11-01 |website=www.wikisky.org}}] |
| {{nowrap|Brightest}} | Lacaille 8760 | | V= 6.69 | {{see|#List of brightest red dwarfs}}
Also called AX Microscopii. This is the 24th closest star to the Sun, and also intrinsically luminous for red dwarfs, having spectral class M0. | [{{cite magazine |url= http://kencroswell.com/thebrightestreddwarf.html |title= The Brightest Red Dwarf |author= Ken Croswell |date= July 2002 |page= 38 |journal= Sky and Telescope }}][{{cite magazine |url= http://www.skyandtelescope.com/wp-content/uploads/Lalande+21185+Sidebar.pdf |title= Lalande 21185: The Brightest Red Dwarf for the Rest of Us |year= 2013 |author= David Tytell }}] |
| {{nowrap|Youngest}} | See T Tauri star | | | {{see|#List of youngest red dwarfs}} | |
| {{nowrap|Oldest}} | See cool subdwarfs | | | {{see|#List of oldest red dwarfs}} | |