Matches in DBpedia 2016-04 for { ?s ?p "(225312) 1996 XB27, also written as (225312) 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU."@en }
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- (225312)_1996_XB27 abstract "(225312) 1996 XB27, also written as (225312) 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU.".
- Q4542357 abstract "(225312) 1996 XB27, also written as (225312) 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU.".
- (225312)_1996_XB27 comment "(225312) 1996 XB27, also written as (225312) 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU.".
- Q4542357 comment "(225312) 1996 XB27, also written as (225312) 1996 XB27, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit.It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit.Between 1900 and 2200 its closest approach with Earth is more than 0.11 AU.".