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Stellar HostProfile

DMPP-4

F5-F8 V • 25.33 pc

Records

5

literature rows

Planets

1

system count

References

6

distinct source labels

HIP: HIP 96258TIC: TIC 26884478HD: HD 184960

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: Barnes et al. 2023 • System source: TICv8

Temperature

6400 K

6266 to 6400

3 values • 3 distinct

Mass

1.25 Msun

1.22 to 1.30

3 values • 3 distinct

Radius

1.38 Rsun

1.38 to 1.42

3 values • 3 distinct

Age

2.15 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.46 log(Lsun)

0.43 to 0.46

3 values • 3 distinct

Distance

25.33 pc

single adopted value

5 values • 1 distinct

Spectral Type

F5-F8 V

Multiple classifications reported

F5 (1), F5-F8 V (1), F7V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.38 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

DMPP-4

1.38 R☉

System Layout

Known planets

1 planets linked to this host

DMPP-4 b

Radial Velocity

◌

Discovery

2023

Period

3.50 days

Radius

—

Mass

12.20 M⊕

Eq. Temp

—

DMPP-4 b: A Close-Orbiting Planet Around a Hotter, Larger Star

DMPP-4 is a single-star system 82.6 light-years away. Its star has a spectral type of F5-F8 V, with an age of 2.15 billion years, a mass of 1.25 solar masses, a radius of 1.38 solar radii, and a temperature of 6400 K. Each of these measured properties places the star above the Sun: it is more massive, larger, and hotter.

One planet is known around DMPP-4. DMPP-4 b was found in 2023 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. The planet has a minimum mass of 12.2 Earth masses, larger than Earth's, and an orbital period of 3.5 days. That minimum mass is a lower bound on the planet's true mass, not an exact value.

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Stellar refs

5

System refs

1

Distancestable

5 values • 1 distinct

Parallaxstable

5 values • 1 distinct

Temperaturedisputed

3 values • 3 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

3 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typedisputed

3 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—————F525.33Cannon & Pickering 1918TICv8
——————25.33Nordstrom et al. 2004TICv8
6275.11.221.39—0.43—25.33TICv8TICv8
62661.301.42—0.45F7V25.33Turnbull 2015TICv8
64001.251.382.150.46F5-F8 V25.33Barnes et al. 2023TICv8