8589 Stellaris
Facts
24 properties- Instance of
- asteroid
- Follows
- 8588 Avosetta[7]
- Followed by
- 8590 Pygargus[8]
- Apoapsis
- 2.364 astronomical unit, 2.363178383741212 astronomical unit
- Argument of periapsis
- 51.62919 degree, 51.71772815108793 degree
- Discoverer or inventor
- Cornelis Johannes van Houten, Ingrid van Houten-Groeneveld, Tom Gehrels[2][3][4]
- Epoch
- November 21, 2025
- Longitude of ascending node
- 340.26395 degree, 340.1465728228687 degree
- Mean anomaly
- 175.93886 degree, 298.4349377393278 degree
- Minor planet group
- asteroid belt[9]
- Named after
- Eurasian Bittern[6]
- Periapsis
- 2.0482341 astronomical unit, 2.048026750256065 astronomical unit
- Rotation period
- 5.37 hour
- Semi-major axis of an orbit
- 2.2060356 astronomical unit, 2.205602566998639 astronomical unit
- Site of astronomical discovery
- Palomar Observatory[5]
- Time of discovery or invention
- September 24, 1960[13]
- Time of periapsis
- 2,461,205.1073058834 Julian day
- Freebase ID
- /m/03ygtb1
- JPL Small-Body Database SPK-ID
- 20008589
- Minor Planet Center body ID
- 8589
0 sources
Summary
8589 Stellaris is an asteroid[1].
Body
Works and Contributions
Credited discoveries include Cornelis Johannes van Houten[2], an astronomer[24], 1920–2002[25], of Kingdom of the Netherlands[26], specialised in astronomy[27]; Ingrid van Houten-Groeneveld[3], an astronomer[28], 1921–2015[29], of Kingdom of the Netherlands[30], specialised in astronomy[31]; and Tom Gehrels[4], an astronomer[32], 1925–2011[33], of Kingdom of the Netherlands[34], awarded the Masursky Award[35], specialised in astronomy[36].