Statements (64)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:nebula
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:NGC_1300
|
| gptkbp:aftermath |
studied through simulations
|
| gptkbp:apparent_magnitude |
approximately 16.5
|
| gptkbp:associated_with |
the Tarantula Nebula
|
| gptkbp:bomb_load |
estimated at 1-2 x 10^51 ergs
|
| gptkbp:characteristics |
analyzed for physical properties
|
| gptkbp:collaborations |
gptkb:NASA_and_ESA
international astronomical community published in scientific journals ongoing with multiple institutions formed to analyze data |
| gptkbp:community_engagement |
captured the attention of amateur astronomers
|
| gptkbp:conference |
discussed in various forums
|
| gptkbp:conservation_efforts |
gptkb:nebula
complex and evolving growing over time contains heavy elements estimated to be several years old |
| gptkbp:contains |
gptkb:nebula
|
| gptkbp:contributed_to |
of stellar death processes
understanding of cosmic nucleosynthesis |
| gptkbp:discovered_by |
gptkb:Hubble_Space_Telescope
|
| gptkbp:distance |
approximately 160,000 light-years
|
| gptkbp:education |
used as a case study in astronomy courses
|
| gptkbp:events |
conducted in multiple wavelengths
ongoing to this day |
| gptkbp:expansion_plans |
approximately 5000 km/s
|
| gptkbp:future_plans |
identified based on findings.
|
| gptkbp:has_spectral_type |
analyzed for chemical composition
hydrogen-rich spectrum |
| gptkbp:hosts |
gptkb:NGC_1978
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 2007 A
|
| gptkbp:impact |
in the field of astrophysics
enhanced knowledge of supernova mechanisms provides insights into the expansion of the universe |
| gptkbp:influenced_by |
in the field of supernova research
|
| gptkbp:instrumentation |
provided insights into elemental abundances
|
| gptkbp:is_observed_in |
various telescopes
showed strong hydrogen lines continue to yield new data |
| gptkbp:is_reflected_in |
observed in subsequent years
|
| gptkbp:length |
2007-01-09
|
| gptkbp:lighting |
observed in subsequent years
used to estimate parameters characteristic of Type II supernovae reached in 2007 revealed important characteristics showed a rapid rise and decline |
| gptkbp:located_in |
gptkb:the_Large_Magellanic_Cloud
|
| gptkbp:next_event |
planned to study its evolution
|
| gptkbp:power_output |
about 10^51 ergs
|
| gptkbp:related_model |
developed to explain observations
|
| gptkbp:research |
advanced due to its study
launched to monitor the remnant presented for astronomers shared with the global scientific community |
| gptkbp:research_focus |
helps understand core-collapse supernovae
|
| gptkbp:significance |
important for studying stellar evolution
|
| gptkbp:species |
monitored over time
|
| gptkbp:storage |
collected over several years
|
| gptkbp:type |
gptkb:Type_II_supernova
|
| gptkbp:year_created |
2007-01-09
|