|
gptkbp:instance_of
|
gptkb:star
|
|
gptkbp:average_temperature
|
approximately 6000 K
|
|
gptkbp:contains
|
gptkb:hydrogen
helium
|
|
gptkbp:examines
|
gptkb:Research_Institute
physical properties
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Local Interstellar Cloud
|
|
gptkbp:is_adjacent_to
|
G-cloud
S-cloud
|
|
gptkbp:is_affected_by
|
galactic dynamics
|
|
gptkbp:is_analyzed_in
|
chemical composition
its dynamics
|
|
gptkbp:is_associated_with
|
gptkb:observatory
the solar system's motion
|
|
gptkbp:is_characterized_by
|
low density
low metallicity
|
|
gptkbp:is_connected_to
|
the heliosphere
other interstellar clouds
the galactic center
|
|
gptkbp:is_considered_as
|
a region of star formation
|
|
gptkbp:is_described_as
|
various models
various theories
|
|
gptkbp:is_documented_in
|
gptkb:literary_work
|
|
gptkbp:is_expected_to
|
about 30 light-years across
|
|
gptkbp:is_explored_in
|
gptkb:spacecraft
|
|
gptkbp:is_home_to
|
cosmic rays
|
|
gptkbp:is_influenced_by
|
gptkb:engine
gptkb:supernova_remnants
magnetic fields
|
|
gptkbp:is_inhabited_by
|
various molecules
|
|
gptkbp:is_linked_to
|
the formation of new stars
|
|
gptkbp:is_located_near
|
gptkb:Orion_Arm
|
|
gptkbp:is_observed_in
|
gptkb:observatory
radio telescopes
|
|
gptkbp:is_part_of
|
solar neighborhood
interstellar matter
the interstellar medium of the Milky Way
the local galactic environment
the local interstellar medium
|
|
gptkbp:is_studied_in
|
astrophysics
its role in galactic ecology
its impact on solar activity
|
|
gptkbp:is_subject_to
|
stellar radiation
|
|
gptkbp:is_surrounded_by
|
gptkb:interstellar_medium
|
|
gptkbp:located_in
|
gptkb:Milky_Way_Galaxy
|
|
gptkbp:map
|
space telescopes
galactic surveys
|
|
gptkbp:part_of
|
gptkb:Local_Bubble
|
|
gptkbp:population
|
about 0.1 atoms per cubic centimeter
|
|
gptkbp:bfsParent
|
gptkb:Local_Bubble
|
|
gptkbp:bfsLayer
|
4
|