대광고 고1 · D-3 근거 회수 기록 5문항 · 모의고사형

An observatory keeps a log of cloudy nights as carefully as nights when stars can be measured. A visitor wonders why a record should include occasions when nothing was observed. The astronomer explains that the gaps affect what can be inferred from the measurements. If a variable star seems to brighten between two observations, a long cloudy interval may conceal when the change began or whether it briefly reversed. The missing nights are not additional measurements of the star, but they are information about the coverage of the record. Without them, a sequence of isolated observations may look more continuous than it was. Recording an interruption preserves the difference between a stable pattern actually observed and a smooth pattern imagined across an unobserved interval.

An observatory keeps a log of cloudy nights as carefully as nights when stars can be measured. A visitor wonders why a record should include occasions when nothing was observed. The astronomer explains that the gaps affect what can be inferred from the measurements. If a variable star seems to brighten between two observations, a long cloudy interval may conceal when the change began or whether it briefly reversed. The missing nights are not additional measurements of the star, but they are information about the coverage of the record. Without them, a sequence of isolated observations may look more continuous than it was. Recording an interruption preserves the difference between a stable pattern actually observed and a smooth pattern imagined across an unobserved interval.

An observatory keeps a log of cloudy nights as carefully as nights when stars can be measured. A visitor wonders why a record should include occasions when nothing was observed. The astronomer explains that the gaps affect what can be inferred from the measurements. If a variable star seems to brighten between two observations, a long cloudy interval may conceal when the change began or whether it briefly reversed. The missing nights are not additional measurements of the star, but they are information about the coverage of the record. Without them, a sequence of isolated observations may look more continuous than it was. Recording an interruption preserves the difference between a stable pattern actually observed and a smooth pattern imagined across an unobserved interval.

An observatory keeps a log of cloudy nights as carefully as nights when stars can be measured. A visitor wonders why a record should include occasions when nothing was observed. The astronomer explains that the gaps affect what can be inferred from the measurements. If a variable star seems to brighten between two observations, a long cloudy interval may conceal when the change began or whether it briefly reversed. The missing nights are not additional measurements of the star, but they are information about the coverage of the record. Without them, a sequence of isolated observations may look more continuous than it was. Recording an interruption preserves the difference between a stable pattern actually observed and a smooth pattern imagined across an unobserved interval.

An observatory keeps a log of cloudy nights as carefully as nights when stars can be measured. A visitor wonders why a record should include occasions when nothing was observed. The astronomer explains that the gaps affect what can be inferred from the measurements. If a variable star seems to brighten between two observations, a long cloudy interval may conceal when the change began or whether it briefly reversed. The missing nights are not additional measurements of the star, but they are information about the coverage of the record. Without them, a sequence of isolated observations may look more continuous than it was. Recording an interruption preserves the difference between a stable pattern actually observed and a smooth pattern imagined across an unobserved interval.