(Q89406255)

SIMBAD

275 Candidates and 149 Validated Planets Orbiting Bright Stars in K2 Campaigns 0–10

3 references

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

K2-198c

2 references

Ecliptic Plane Input Catalog

EPIC 212768333c

catalog

2 references

Ecliptic Plane Input Catalog

EPIC 212768333.01

catalog

2 references

time of discovery or invention

TIC 135043332c

1 reference

July 2019

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

2 references

inferred from equatorial coordinates

constellation

Virgo

1 reference

based on heuristic

parent astronomical body

3 references

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

object stated in reference as

K2-198

object stated in reference as

2MASS J13152252-0627535

orbital inclination

86.494±0.268 degree

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

orbital period

3.3596055±0.000004 day

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

3.3596055±0.0000021 day

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

semi-major axis of an orbit

0.03077±0.00058 astronomical unit

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

declination component of proper motion

parallax

9.0163±0.0704 milliarcsecond

2 references

−21.893±0.063 milliarcsecond per year

2 references

right ascension component of proper motion

−36.688±0.094 milliarcsecond per year

2 references

1.423±0.081 Earth radius

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

0.127±0.007 Jupiter radius

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

3 references

right ascension

198.8436817 degree

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?

declination

−6.4649888 degree

1 reference

Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?