Artist impression of HD 81040 b exoplanet
Confirmed Exoplanet Discovered 2005

HD 81040 b

A gas giant orbiting the g-type yellow (sun-like) HD 81040, located approximately 112.3 light-years from Earth.

Image: Wikimedia Commons · CC BY-SA 3.0 igo · ESA/Gaia/DPAC

Key parameters at a glance

  • A radius of 12.60 Earth radii
  • A mass of 2,301.08 Earth masses
  • Surface gravity around 14.49 g
  • An orbital period of 1,002.700 days
  • Semi-major axis 1.9460 AU
  • Distance from Earth 112.31 light-years
  • Earth Similarity Index 0.427
  • Travel time at Voyager 1 speed 1,980,567 years

Context from the literature

HD 81040 b is a massive gas giant exoplanet that orbits the star HD 81040, discovered in 2005 by radial velocity. Its orbital period is just over 1000 days. It has a semimajor axis of about 1.95 AU, and its orbit is quite eccentric, at a little over 0.5.

Excerpted from Wikipedia · full article

HD 81040 b Planet Profile

Physical Specs

Radius
12.60 R⊕
Radius (Jupiter)
1.130 R♃
Mass
2,301.08 M⊕
Mass (Jupiter)
7.240 M♃
Density
6.32 g/cm³
Surface Gravity
14.49 g (Earth)

Classification

Planet Type

Gas Giant

ESI Score 0.427
HZ Position Unknown
Controversial No

Discovery

Year 2005
Method Radial Velocity
Facility Multiple Observatories
Telescope Multiple Telescopes

Size rank in cohort

Rank by radius

#1179of 1771

top 66.5%

This planet

12.60R⊕

Gas Giant median

13.52R⊕

Nearest-size peers

Metric Earth HD 81040 b Jupiter
Radius (R⊕)1.0012.6011.21
Mass (M⊕)1.002,301.08317.83
Density (g/cm³)5.516.321.33
Surface Gravity (g)1.0014.492.53
Insolation (S⊕)1.000.037

Alternative Mass Estimates

Method Value Interpretation
Best measured mass 2,301.078 M⊕ Direct mass measurement (not derived).
Minimum mass (M sin i) 2,183.481 M⊕ Lower bound from radial-velocity fitting.

Star Catalogue Identifiers

HD

HD 81040

HIP

HIP 46076

TIC

TIC 414965996

Gaia DR2

Gaia DR2 637329067477530368

Gaia DR3

Gaia DR3 637329067477530368

System

HD 81040

Percentile among Gas Giant cohort

Radius 12.600 R⊕ · percentile 31 / cohort 1771
Mass 2,301.078 M⊕ · percentile 82 / cohort 1747
Orbital period 1,002.70 d · percentile 77 / cohort 1533
Distance 34.43 pc · percentile 10 / cohort 1759
ESI 0.427 · percentile 93 / cohort 1771

Orbit & Habitability

Orbital Dynamics

Period
1,002.700 days
Semi-major axis
1.9460 AU
Eccentricity
0.525
Inclination
73.00 °

Year Length

A year here lasts about 2.75 Earth years on a highly eccentric trajectory at a mean orbital distance of 1.9460 AU.

Eq. Temperature

 

Insolation (S⊕)

Earth = 1.00

Earth Similarity (ESI)

0.427

0 = alien, 1 = Earth-identical

Detection Signatures

Radial velocity

Stellar wobble has been measured spectroscopically.

Astrometry

Positional wobble of the host star was measured.

Discovery Paper

Primary reference

Sozzetti et al. 2006

Instrument

Multiple Instruments

Publication

2006-04

Observation locale

Ground

Host System: HD 81040

Spectral Class

G-type yellow (Sun-like)

Effective Temperature

5,755 K — cooler than the Sun (5,778 K)

Estimated Age

1.79 Gyr — younger than the Sun (4.6 Gyr)

Stellar Radius

0.910 R☉

Stellar Mass

0.990 M☉

Metallicity [Fe/H]

-0.04

Extended Stellar Properties

Surface gravity (log g)

4.540 dex

Stellar density

1.883 g/cm³

Systemic radial velocity

49.25 km/s

Rotational v·sin i

2.00 km/s

Rotation period

15.98 days

Activity index (log R'HK)

-4.710

Metallicity ratio

[Fe/H]

Distance
34.43 parsec
Light-years 112.31 ly
V-band magnitude
7.72 mag
Voyager-speed travel 1,980,567 yr

Multi-band Host Photometry — 12 bands

6.18.48.38B7.72V7.56Gaia8.27Kepler7.13TESS6.51J6.27H6.16K6.17W16.09W26.19W36.11W4

Astrometric Data

Parallax

29.012 mas

Total Proper Motion

155.512 mas/yr

PM Right Ascension

-151.26 mas/yr

PM Declination

36.12 mas/yr

Galactic Cartesian (pc)

x = -0.728 · y = 0.591 · z = 0.348

Equatorial (J2000)

RA 140.94550° · Dec 20.36461°

Galactic ℓ, b

209.363° · 42.326°

Ecliptic λ, β

136.934° · 4.837°

HTM-20 index

605949009

Observation Record

Photometric series

1

RV measurements

2

Archive notes

2

Wikipedia → Image: Wikimedia Commons · ESA/Gaia/DPAC · CC BY-SA 3.0 igo

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