(Q113600492)

mass

0.13 Jupiter mass

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

0.0434±0.0299 Jupiter mass

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

catalog code

TOI-1670b

catalog

TESS Object of Interest

2 references

time of discovery or invention

TOI-1670.02

catalog

TESS Object of Interest

1 reference

TIC 441739020b

1 reference

TIC 441739020.02

1 reference

March 2022

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

2 references

inferred from equatorial coordinates

constellation

Draco

1 reference

based on heuristic

parent astronomical body

3 references

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

object stated in reference as

TOI-1670

object stated in reference as

TOI-1670

argument of periapsis

163.6±53.7 degree

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

orbital eccentricity

0.59±0.26

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

orbital inclination

86.87±1.16 degree

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

orbital period

10.98462±0.00051 day

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

semi-major axis of an orbit

0.103±0.002 astronomical unit

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

parallax

6.0224±0.0133 milliarcsecond

2 references

Gaia Early Data Release 3

declination component of proper motion

SIMBAD

4.923±0.018 milliarcsecond per year

2 references

Gaia Early Data Release 3

right ascension component of proper motion

SIMBAD

−6.007±0.018 milliarcsecond per year

2 references

Gaia Early Data Release 3

SIMBAD

radius

2.06±0.19 Earth radius

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

0.1838±0.017 Jupiter radius

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

3 references

right ascension

259.0172522 degree

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

declination

72.1611806 degree

1 reference

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration