4:["$","div",null,{"className":"min-h-screen bg-white flex flex-col","children":[["$","div",null,{"className":"px-6 pt-6 pb-4 border-b border-gray-100","children":[["$","div",null,{"className":"flex items-center gap-1.5 text-xs text-gray-400 mb-4","children":[["$","a",null,{"href":"/","className":"hover:text-[#26a69a] transition-colors","children":"Market"}],["$","span",null,{"children":"›"}],["$","span",null,{"className":"text-gray-600","children":"300P/Catalina"}]]}],["$","div",null,{"className":"text-[10px] text-gray-400 uppercase tracking-widest mb-1","children":"Company Profile"}],["$","h1",null,{"className":"text-2xl font-bold text-gray-900","children":"300P/Catalina"}],null]}],["$","div",null,{"className":"flex-1 px-6 py-6","children":[["$","p",null,{"className":"text-sm text-gray-600 leading-relaxed mb-8","children":"300P/Catalina is a periodic, near-Earth comet in the Solar System with an orbital period of 4.4 years. It is the second comet ever listed on the Sentry Risk Table. At 1.4 km (0.87 mi) in diameter, it is one of the largest objects ever listed on the Sentry Risk Table."}],["$","div",null,{"className":"columns-1 md:columns-2 gap-10","children":[["$","div","0",{"className":"mb-8 break-inside-avoid","children":[["$","div",null,{"className":"text-xs font-semibold text-gray-400 uppercase tracking-wide mb-3 border-b border-gray-100 pb-1","children":"Observational history"}],["$","div",null,{"className":"text-sm text-gray-600 leading-relaxed wiki-content","dangerouslySetInnerHTML":{"__html":"It was discovered on 6 May 2005 as , and listed on the Sentry Risk Table with five virtual impactors starting in 2041. On 17 May 2005 it was designated as comet P/2005 JQ5 (Catalina). It was removed from the Sentry Risk Table on 7 June 2005. It was observed by Arecibo Observatory on 12 June 2005. 300P/Catalina makes close approaches to Earth and has an Earth-MOID of . On 8 June 2036 the comet will pass from Earth. == Meteor shower =="}}]]}],["$","div","1",{"className":"mb-8 break-inside-avoid","children":[["$","div",null,{"className":"text-xs font-semibold text-gray-400 uppercase tracking-wide mb-3 border-b border-gray-100 pb-1","children":"Meteor shower"}],["$","div",null,{"className":"text-sm text-gray-600 leading-relaxed wiki-content","dangerouslySetInnerHTML":{"__html":"300P/Catalina is suspected of being the parent body of the minor June Epsilon Ophiuchids meteor shower. There was an outburst of meteor activity from 19 June 2019 until 26 June 2019 when 88 June epsilon Ophiuchids were detected by the Cameras for Allsky Meteor Surveillance (CAMS) network. The June epsilon Ophiuchids created 50% of the fireball detections in the period 22–24 June. This outburst offers evidence of past activity of 300P/Catalina. The radiant is near 16:21 (245.2) -7.4 in the constellation of Ophiuchus. The June epsilon Ophiuchids radiate from a very large scattered radiant area and may be related to a number of other minor showers that have been identified. The meteors have a velocity of around 14 km/s. == References =="}}]]}]]}],["$","div",null,{"className":"mt-8 pt-4 border-t border-gray-100","children":["$","a",null,{"href":"https://en.wikipedia.org/wiki/300P%2FCatalina","target":"_blank","rel":"noopener noreferrer","className":"text-xs text-gray-400 hover:text-gray-600 transition-colors","children":"Source: Wikipedia ↗"}]}]]}],"$Lf"]}]