Title: 12 Aquarii
Content:  12 Aquarii is a triple star system in the zodiac constellation of Aquarius. 12 Aquarii is the Flamsteed designation. It is visible to the naked eye as a dim star with an apparent visual magnitude of 5.67. Parallax measurements by Hipparcos puts it at a distance of some 500 light-years, or 150 parsecs away. The system is moving further from the Earth with a heliocentric radial velocity of +1.1 km/s. The magnitude 5.88 primary, component A, is itself a binary star with a separation of 0.05 arcsecond–0.07 arcsecond and an orbital period of around 6760 days. The brighter member of this duo is a G-type bright giant with a stellar classification of G4 II and 2.6 times the mass of the Sun. Its companion is an early A-type star with double the mass of the Sun. The tertiary component B is magnitude 7.55 A-type main-sequence star at a separation of 2.44 arcsecond from the primary.
Title: 12 Lacertae
Content:  12 Lacertae is a wide binary star system in the northern constellation of Lacerta, located roughly 1,090 light years away from the Sun based on parallax. It is visible to the naked eye as a dim, blue-white hued point of light with a baseline apparent visual magnitude of 5.23. The system is drifting closer to the Earth with a mean heliocentric radial velocity of –12.5. It is a probable member of the I Lacertae OB association (Lac OB1). The primary component is a Beta Cephei variable with a stellar classification of B1.5III, matching a B-type star with the luminosity class of a giant star. It has been known to be variable for more than a century 
Title: Lambda Herculis
Content:  Lambda Herculis has apparent magnitude +4.4 spectral class K4III, indicating that it is a red giant with a temperature of 4,070 K. Visually it has an absolute magnitude of &minus;0.86, meaning it is nearly 200 times brighter than the sun, but its bolometric luminosity across all wavelengths is. In 1783, English-German astronomer William Herschel described the solar apex, the point in sky towards which the Solar System is moving; using data from double stars, he identified this position as close to Lambda Herculis. Today it is known the solar apex is not so close to this star, however it is only 10° away from the position currently accepted (in Hercules, southwest of Vega).
Title: 12 Lyncis
Content:  12 Lyncis, abbreviated 12 Lyn, is a triple star system in the constellation Lynx. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.87. When seen through a telescope, it can be separated into three stars: two components with magnitudes 5.4 and 6.0 that lie at an angular separation by 1.8″ (as of 1992) and a yellow-hued star of magnitude 7.2 at a separation of 8.6″ (as of 1990). The orbit of the two brighter stars is not known with certainty, but appears to have a period of somewhere around 700 to 900 years. The pair have a projected separation of 128 AU. Parallax indicates the system is 210 light years distant from Earth.
Title: Lambda Leporis
Content:  Lambda Leporis, which is the Latinized form of λ Leporis, is a solitary, blue-white hued star in the southern constellation of Lepus. It is visible to the naked eye with an apparent visual magnitude of +4.29. Based upon an annual parallax shift of 3.83 mas, it is estimated to lie roughly 850 light years from the Sun. Relative to its neighbors, this star has a peculiar velocity of 16.3 km/s. It is a member of the Orion OB1 association (Ori OB1), and it has been identified as a high-velocity runaway star. This is a massive, B-type main-sequence star with a corrected stellar classification of B0.5 V. It is an estimated eight million years old and is spinning with a projected rotational velocity of 30 km/s. This star has around 15 times the mass of the Sun and 4.5 times the Sun's radius. It is radiating 15,488 times the Sun's luminosity from its photosphere at an effective temperature of 30,400 K.
Title: 12 Lacertae
Content:  the luminosity of the Sun from its photosphere at an effective temperature of 23,809 K. The estimated rotational velocity of the primary at the equator is 52 km/s; about 10% of its break-up velocity. However, seismic models suggest the core region is rotating much more rapidly with a rotational velocity of up to 100 km/s, and thus the star is undergoing differential rotation. The companion is an A-type main-sequence star with a stellar classification of A3V and visual magnitude 9.2. As of 2008, it had an angular separation of 69 arcsecond from the primary. There is a faint infrared nebulosity at a separation of 0.19 pc from the pair that is most likely a bow shock.
Title: Theta Leporis
Content:  Theta Leporis, Latinized from θ Leporis, is a solitary, white-hued star in the southern constellation of Lepus. It has an apparent visual magnitude of 4.67, making it bright enough to be viewed with the naked eye. Based upon an annual parallax shift of 18.88 mas as measured from Earth, the system is located roughly 173 light years from the Sun. The star made its closest approach about 1.6 million years ago when it came within 9.0 pc of the Sun. This is an ordinary A-type main-sequence star with a stellar classification of A0 V and an age of about 207 million years. It is rotating rapidly with a projected rotational velocity of 207 km/s. This is giving the star an oblate shape with an equatorial bulge that is an estimated 10% larger than the polar radius. It has an estimated 2.35 times the mass of the Sun and is radiating 41 times the Sun's luminosity from its photosphere at an effective temperature of around 10,453 K.
Title: 21 Lyncis
Content:  21 Lyncis is a single star in the northern constellation of Lynx. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.61. The star is located at a distance of about 274 light years away from the Sun, based on parallax. It is moving further away from the Earth with a heliocentric radial velocity of around +27 km/s. This object is an ordinary A-type main-sequence star with a stellar classification of A0.5Vs, where the 's' suffix indicates "sharp" lines in the spectrum, usually due to slow rotation. It is about 272 million years old with a projected rotational velocity of 18 km/s. The star has 2.22 times the mass of the Sun and is radiating 102 times the luminosity of the Sun from its photosphere at an effective temperature of 9,692 K.
Title: 12 Persei
Content:  12 Persei (12 Per) is a double-lined spectroscopic binary star system in the northern constellation Perseus. Its combined apparent magnitude is 4.94, which means it can be viewed with the naked eye. Based upon parallax measurements, this system is about 79 light years away from the Sun. The magnitude difference between the two components is estimated to be 0.51. Based upon this, the primary has a mass around 138% of the Sun, 155% of the Sun's radius, and shines with three times the Sun's luminosity. The smaller secondary component is also larger than the Sun, with 124% of the Sun's mass, 131% of the radius of the Sun, and has 186% of the Sun's luminosity. The stellar classification of the primary is F9 V, which suggests it is an F-type main sequence star. The pair have an estimated age of just over a billion years. The pair orbit each other with a period of 331 days and an eccentricity of 0.663. The semimajor axis of their orbit is 1.27 AU, which means the inner stability radius for a hypothetical planet orbiting the pair would be at 4.35 AU. This lies outside the habitability zone for this system.
Title: 11 Lacertae
Content:  11 Lacertae is a star in the northern constellation of Lacerta. It is visible to the naked eye as a faint orange-hued star with an apparent visual magnitude of 4.46. It lies at a distance of about 333 light years and has an absolute magnitude -0.54. The object is moving closer to the Earth with a heliocentric radial velocity of −10.9 km/s. This is an evolved giant star with a stellar classification of K2.5 III. It is a red clump giant, meaning it is fusing helium in its core after passing through the red giant branch. The star is 3.2 billion years old with 1.38 times the mass of the Sun and has expanded to 27.7 times the Sun's radius. It is radiating 204 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,352 K.

Question: Verify the following claims with "True" or "False": The temperature of 120 Lachesis is 171.0 (kelvins) and its apoapsis is 511592000.0 km.
Answer: False