KELT-24#Planetary system

{{Short description|Star in Ursa Major}}

{{Starbox begin}}

{{Starbox observe 2s

| epoch = J2000.0

| constell = Ursa Major

| component1 = KELT-24

| ra1 = {{RA|10|47|38.35063}}

| dec1 = {{DEC|+71|39|21.1525}}

| appmag_v1 = 8.33

| component2 = KELT-24B

| ra2 = {{RA|10|47|38.38264}}

| dec2 = {{DEC|+71|39|19.1482}}

| appmag_v2 =

}}

{{Starbox character

| component1 = KELT-24

| class = F5

| type = main sequence

| variable = planetary transit

| component2 = KELT-24B

| class2 = M + M?

| type2 = main sequence

| variable2 = eclipsing

}}

{{Starbox astrometry

| component1 = KELT-24

| radial_v = {{val|-5.54|0.24}}

| prop_mo_ra = −56.061

| prop_mo_dec = −34.526

| pm_footnote =

| parallax = 10.3218

| p_error = 0.0180

| parallax_footnote =

| absmag_v = +3.47

| component2 = KELT-24B

| radial_v2 =

| prop_mo_ra2 = −49.897

| prop_mo_dec2 = −37.516

| pm_footnote2 =

| parallax2 = 10.6799

| p_error2 = 0.0892

| parallax_footnote2 =

| absmag_v2 =

}}

{{Starbox detail

| source =

| component1 = KELT-24

| mass = 1.31

| radius = 1.51

| luminosity = 3.54

| temperature = 6,437

| gravity = 4.19

| metal_fe = 0.17

| rotation = ~4 days

| rotational_velocity = 19.7

| age_gyr = 2.8

}}

{{Starbox detail|no_heading=y

| component1 = B

| mass = 0.52

| radius = 0.48

| luminosity = 0.037

| temperature = 3,630

| gravity = 4.78

| metal_fe = 0.30

| rotation =

| rotational_velocity =

| age_gyr = 2.8

| component2 = C

| mass2 = 0.51

| radius2 = 0.49

| luminosity2 = 0.038

| temperature2 = 3,640

| gravity2 = 4.77

| metal_fe2 = −0.31

| rotation2 =

| rotational_velocity2 =

| age_gyr2 = 2.8

}}

{{starbox catalog

|names=MASCARA-3, KELT-24, HD 93148, HIP 52796

}}

{{Starbox reference

| Simbad = HD+93148

| Simbad2 = HD+93148B |sn2 = B

}}

{{Starbox end}}

KELT-24 (HD 93148, MASCARA-3) is a multiple star system in the constellation Ursa Major at a distance of approximately 316 light-years (about 96.9 parsecs) from Sun. The apparent magnitude of the primary star is +8.33. The star's age is estimated to be about 2.8 billion years. As an F-type main-sequence star, it is similar to the Sun, but slightly hotter, larger, and more luminous.

KELT-24 has a single known exoplanet, a hot Jupiter only {{solar radius|11|link=y}} from the star.

Nomenclature

This star was first catalogued in the Henry Draper Catalogue as HD 93148. The Henry Draper Catalogue gave stars visible to the naked eye in suitable conditions a designation, indicating that this star can be seen with the naked eye. But in 2019, the Multi-site All-Sky Camera and the Kilodegree Extremely Little Telescope announced the discovery of the exoplanet KELT-24b/MASCARA-3b around this star. Thus, it is most commonly known as KELT-24, although the star is sometimes catalogued as MASCARA-3.

The common proper motion companion is referred to as HD 93148B or KELT-24B, or KELT-24BC when it is being treated as a spectroscopic binary.

Star system

KELT-24 is an 8th-magnitude F-type star with a faint companion separated by {{val|2|ul="}}. The companion is over-luminous for a normal star of its colour and is suspected to be a binary consisting of two red dwarfs.

KELT-24 is a yellow-white star with a spectral class of F5. Its mass is about {{Solar mass|1.3|link=y}}, its radius is about {{Solar radius|1.5|link=y}}, and its luminosity is about {{Solar luminosity|3.5|link=y}}. Its effective temperature is about {{val|fmt=commas|6437|ul=K}}. An age of 2.8 billion years has been calculated, but the 68% confidence interval ranges from 2.0 to 6.9 billion years. Age estimates in the original discovery papers were 0.78 and 2.8 billion years respectively.

KELT-24B, or KELT-24BC when both components are being referred to, is suspected of being an eclipsing binary although only a single "transit-like event" has been observed. The best model fit is two near-identical red dwarfs each with a mass about half the Sun's and a luminosity less than 4% of the Sun's.

Planetary system

In 2019, the discovery of the Hot Jupiter type planet KELT-24b/MASCARA-3b was announced by the Multi-site All-Sky CAmeRA and the Kilodegree Extremely Little Telescope. TESS data confirmed that no additional companions are orbiting this star.

{{Orbitbox planet begin

|name= KELT-24

}}

{{Orbitbox planet

| exoplanet = b

| mass = 4.6

| semimajor = 0.0501

| radius = 1.1

| eccentricity = 0.032

| period = 5.5515

| inclination = 89.7

}}

{{Orbitbox end}}

References

{{reflist|refs=

{{cite simbad |title=KELT-24 |access-date=2025-05-27 }}

{{Cite Gaia DR3|1076970406751899008}}

{{Cite Gaia DR3|1076970406752355584}}

{{cite XHIP|52796}}

{{cite journal |bibcode=1993yCat.3135....0C |title=VizieR Online Data Catalog: Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989) |last1=Cannon |first1=A. J. |last2=Pickering |first2=E. C. |journal=Vizier Online Data Catalog |date=1993 }}

{{cite journal|bibcode=2000A&A...355L..27H|title=The Tycho-2 catalogue of the 2.5 million brightest stars|journal=Astronomy and Astrophysics|volume=355|pages=L27|last1=Høg|first1=E.|last2=Fabricius|first2=C.|last3=Makarov|first3=V. V.|last4=Urban|first4=S.|last5=Corbin|first5=T.|last6=Wycoff|first6=G.|last7=Bastian|first7=U.|last8=Schwekendiek|first8=P.|last9=Wicenec|first9=A.|year=2000}}

{{cite journal|arxiv=2010.11977|year=2020|title=Search for Planets in Hot Jupiter Systems with Multi-Sector TESS Photometry. I. No Companions in Planetary Systems KELT-18, KELT-23, KELT-24, Qatar-8, WASP-62, WASP-100, WASP-119, and WASP-126|volume=70 |issue=3 |doi=10.32023/0001-5237/70.3.2 |last1=Maciejewski |first1=G. |journal=Acta Astronomica |page=181 |bibcode=2020AcA....70..181M |s2cid=225061977 }}

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{{cite web |title=Exoplanet-catalog |url=https://exoplanets.nasa.gov/exoplanet-catalog/7472/kelt-24-b/ |website=Exoplanet Exploration: Planets Beyond our Solar System |date=13 September 2019 |access-date=10 September 2023 |language=en}}

{{cite journal |bibcode=2024AJ....168..118G |title=Trials and Tribulations in the Reanalysis of KELT-24 b: A Case Study for the Importance of Stellar Modeling |last1=Giovinazzi |first1=Mark R. |last2=Cale |first2=Bryson |last3=Eastman |first3=Jason D. |last4=Rodriguez |first4=Joseph E. |last5=Blake |first5=Cullen H. |last6=Stassun |first6=Keivan G. |last7=Vanderburg |first7=Andrew |last8=Kunimoto |first8=Michelle |last9=Kraus |first9=Adam L. |last10=Twicken |first10=Joseph |last11=Beatty |first11=Thomas G. |last12=Dedrick |first12=Cayla M. |last13=Horner |first13=Jonathan |last14=Johnson |first14=John A. |last15=Johnson |first15=Samson A. |last16=McCrady |first16=Nate |last17=Plavchan |first17=Peter |last18=Sliski |first18=David H. |last19=Wilson |first19=Maurice L. |last20=Wittenmyer |first20=Robert A. |last21=Wright |first21=Jason T. |last22=Johnson |first22=Marshall C. |last23=Rose |first23=Mark E. |last24=Cornachione |first24=Matthew |journal=The Astronomical Journal |date=2024 |volume=168 |issue=3 |page=118 |doi=10.3847/1538-3881/ad55ec |doi-access=free |arxiv=2406.04288 }}

{{cite journal |bibcode=2019A&A...631A..76H |title=MASCARA-3b. A hot Jupiter transiting a bright F7 star in an aligned orbit |last1=Hjorth |first1=M. |last2=Albrecht |first2=S. |last3=Talens |first3=G. J. J. |last4=Grundahl |first4=F. |last5=Justesen |first5=A. B. |last6=Otten |first6=G. P. P. L. |last7=Antoci |first7=V. |last8=Dorval |first8=P. |last9=Foxell |first9=E. |last10=Fredslund Andersen |first10=M. |last11=Murgas |first11=F. |last12=Palle |first12=E. |last13=Stuik |first13=R. |last14=Snellen |first14=I. A. G. |last15=Van Eylen |first15=V. |journal=Astronomy and Astrophysics |date=2019 |volume=631 |doi=10.1051/0004-6361/201936082 |arxiv=1906.05254 }}

}}