←Back to Stellar Hosts
Stellar HostProfile

HD 21693

Unclassified star • 33.26 pc

Records

8

literature rows

Planets

2

system count

References

9

distinct source labels

HIP: HIP 16085HD: HD 21693TIC: TIC 197792776

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.

Stellar source: TICv8 • System source: TICv8

Temperature

5434.3 K

5430 to 5458.3

4 values • 3 distinct

Mass

0.95 Msun

0.80 to 0.95

3 values • 3 distinct

Radius

0.92 Rsun

0.91 to 0.92

2 values • 2 distinct

Luminosity

-0.17 log(Lsun)

-0.21 to -0.17

4 values • 4 distinct

Distance

33.26 pc

single adopted value

8 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.92 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 21693

0.92 R☉

System Layout

Known planets

2 planets linked to this host

HD 21693 b

Radial Velocity

◌

Discovery

2019

Period

22.68 days

Radius

—

Mass

8.23 M⊕

Eq. Temp

—

HD 21693 c

Radial Velocity

◌

Discovery

2019

Period

53.74 days

Radius

—

Mass

17.37 M⊕

Eq. Temp

—

HD 21693 and Its Two Known Planets

HD 21693 is a G8 V star located 108 light-years away. Its spectral type marks it as a main-sequence dwarf, and it is cooler than the Sun, with a reported temperature of 5430 K. The star's reported radius estimate is smaller than the Sun's, at 0.923 solar radii, and its mass is 0.95 solar masses. Two planets are known to orbit this host.

HD 21693 b and HD 21693 c were both discovered in 2019 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. HD 21693 b has a minimum mass of 8.23 Earth masses, larger than Earth's, and orbits in 22.7 days. HD 21693 c has a minimum mass of 17.4 Earth masses, also larger than Earth's, and orbits in 53.7 days.

Both minimum masses are lower bounds on the planets' true masses. Among the listed planets, HD 21693 b has the shortest year and the smallest minimum mass, while HD 21693 c has the longest year and the largest minimum mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

8

System refs

1

Distancestable

8 values • 1 distinct

Parallaxstable

8 values • 1 distinct

Temperaturedisputed

4 values • 3 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

2 values • 2 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitystable

3 values • 1 distinct

Spectral Typedisputed

4 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—————G8 V33.26Michigan Catalog, Vol. 1TICv8
54300.80——-0.21G8 V33.26Udry et al. 2019TICv8
54300.85——-0.21—33.26Sousa et al. 2008TICv8
—————G533.26Cannon & Pickering 1918TICv8
——————33.26Nordstrom et al. 2004TICv8
5434.30.950.92—-0.17—33.26TICv8TICv8
5458.3—0.91—-0.17—33.26Gaia DR2TICv8
—————G9 IV-V33.26Gray et al. 2006TICv8