061.01 Basics of Navigation Flashcards
At 0000 LMT of an observer the (mean/apparent) Sun is in transit with the observer’s (meridian/anti-meridian).
At 0000 LMT of an observer the (mean) Sun is in transit with the observer’s (anti-meridian).
The maximum difference between geocentric and geodetic latitude occurs at about (…).
The maximum difference between geocentric and geodetic latitude occurs at about (45°N/S).
Astronomical twilight is when the sun is (…)° below the horizon.
Astronomical twilight is when the sun is (18)° below the horizon.
The right visualisation of latitude in the appendix is (Geocentric/Geographic or Geodetic) latitude.
The right visualisation of latitude in the appendix is (Geographic or Geodetic) latitude.
The term Aphelion is the point of the Earth’s orbit (closest/furthest away from) to the sun. The approximate date is (…). At this point the Earth in its orbit reaches the (highest/lowest) speed.
The term Aphelion is the point of the Earth’s orbit (furthest away from) to the sun. The approximate date is (beginning of July). At this point the Earth in its orbit reaches the (lowest) speed.
Nautical twilight is when the sun is (…)° below the horizon.
Nautical twilight is when the sun is (12)° below the horizon.
Lines on a map or charts joining positions with equal magnetic dip are termed (…).
Lines on a map or charts joining positions with equal magnetic dip are termed (isoclinals).
A orthodrome is a (…).
A orthodrome is a (great circle).
The magnetic North Pole seems to rotate around the geographical North Pole at a rate of movement of 1° in (1/5/9/11) years.
The magnetic North Pole seems to rotate around the geographical North Pole at a rate of movement of 1° in (5) years.
State Kepler’s 1st Law
Planets move in elliptic orbits with the sun in one of the foci.
The angle between the plane of the Ecliptic and the plane of Equator is approximately (…)°.
The angle between the plane of the Ecliptic and the plane of Equator is approximately (23.5)°.
State Kepler’s 2nd Law
The radius vector sun-earth sweeps out equal areas in equal time.
The mean Sun is a (visible/fictitious) Sun and the lenght of a day (is constant/varies) throughout the year.
The mean Sun is a (fictitious) Sun and the lenght of a day (is constant) throughout the year.
The relationship between the lenght of day and night, as well as the rate of change of declination of the Sun, changing at the greatest rate is at the (winter and summer solstice/spring and autumn equinox).
The relationship between the lenght of day and night, as well as the rate of change of declination of the Sun, changing at the greatest rate is at the (spring and autumn equinox).
On the Earth’s ellipsoid, one degree of latitude near the poles is (more/less) than 60 NM.
On the Earth’s ellipsoid, one degree of latitude near the poles is (more) than 60 NM.