Statements (61)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:observatory
|
| gptkbp:activities |
develops a coma
develops a tail |
| gptkbp:appearance |
appear sporadically in the inner solar system
|
| gptkbp:archaeological_findings |
noted in ancient records
|
| gptkbp:atmosphere |
contains simple molecules
|
| gptkbp:collaborations |
international teams study comets
|
| gptkbp:color |
often appear dark
|
| gptkbp:composed_of |
ammonia
carbon dioxide water ice organic compounds |
| gptkbp:cultural_impact |
inspired myths and legends throughout history
|
| gptkbp:depicted_in |
visible from Earth
|
| gptkbp:discovered_by |
gptkb:museum
often discovered by telescopes |
| gptkbp:elevation |
affected by gravitational interactions
|
| gptkbp:environment |
found in cold regions of the solar system
|
| gptkbp:example |
gptkb:Comet_Hale-Bopp
gptkb:Comet_67_P/_Churyumov-Gerasimenko |
| gptkbp:formed |
formed in the early solar system
|
| gptkbp:frequency |
discovered frequently due to their visibility
|
| gptkbp:future_plans |
expected to be studied by upcoming missions.
may contain building blocks of life |
| gptkbp:has_luminosity |
increases as it nears the Sun
|
| gptkbp:historical_impact |
some have impacted Earth in the past
|
| gptkbp:historical_significance |
influenced ancient astronomy
|
| https://www.w3.org/2000/01/rdf-schema#label |
C-type comet
|
| gptkbp:impact |
generally low risk to Earth
|
| gptkbp:is_a_tool_for |
spectroscopy used to analyze composition
|
| gptkbp:is_essential_for |
study of solar system formation
|
| gptkbp:is_observed_in |
studied by space missions
|
| gptkbp:is_reflected_in |
low albedo
|
| gptkbp:isotopes |
contains a mixture of ices and dust
|
| gptkbp:length |
can extend millions of kilometers
|
| gptkbp:lifespan |
can last millions of years
|
| gptkbp:location |
outer solar system
|
| gptkbp:mission |
highly elliptical
Rosetta mission studied Comet 67 P |
| gptkbp:notable_event |
gptkb:Comet_1_P/_Halley
|
| gptkbp:notable_feature |
long orbital periods
|
| gptkbp:origin |
gptkb:Kuiper_Belt
gptkb:Cloud_Computing_Service can evolve over time due to solar radiation |
| gptkbp:research |
difficult to observe from Earth due to distance
provides clues about early solar system |
| gptkbp:research_focus |
helps understand organic chemistry in space
|
| gptkbp:research_interest |
targets for future exploration missions
|
| gptkbp:scientific_classification |
one of three main types of comets
|
| gptkbp:size |
can be several kilometers in diameter
sizes vary widely among different comets |
| gptkbp:speed |
can travel at high speeds
|
| gptkbp:tail_type |
always points away from the Sun
tail forms as it approaches the Sun |
| gptkbp:weather_conditions |
can create a plasma tail
|
| gptkbp:bfsParent |
gptkb:Halley_family_of_comets
gptkb:comet_Wild_2 gptkb:Comet_Wild_2 gptkb:Comet_Giacobini-Zinner gptkb:Comet_Halley |
| gptkbp:bfsLayer |
5
|