14 Aquilae

{{Short description|Star in the constellation Aquila}}

{{Starbox begin

| name = 14 Aquilae

}}

{{Starbox observe

| epoch = J2000

| ra = {{RA|19|02|54.50105}}

| dec = {{DEC|-03|41|56.2881}}

| appmag_v = 5.42

| constell = Aquila

}}

{{Starbox character

| type = main sequence

| class = A1 V

| b-v = +0.00

| u-b = –0.07

| variable =

}}

{{Starbox astrometry

| radial_v = {{Val|−39.0|3.7}}

| prop_mo_ra = +15.558

| prop_mo_dec = +2.571

| parallax = 5.4932

| p_error = 0.2368

| parallax_footnote =

| absmag_v = −0.52

}}

{{Starbox detail

| mass = {{Val|3.25|0.05}}

| radius = 2.0

| luminosity = {{Val|213.9|23.8|21.4}}

| temperature = {{Val|9908|46|45|fmt=commas}}

| metal_fe =

| rotational_velocity = 23

| age_myr =

}}

{{Starbox catalog

| names = {{odlist | F=14 Aql | BD=-03°4460 | FK5= | HD=176984 | HIP=93526 | HR=7209 | SAO=142959 | WDS=J19029-0342 }}

}}

{{Starbox reference

|Simbad=14+Aql

}}

{{Starbox end}}

14 Aquilae is a probable spectroscopic binary star system in the equatorial constellation of Aquila. 14 Aquilae is the Flamsteed designation though it also bears the Bayer designation g Aquilae. It is visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 5.42, and it is located at a distance of approximately {{Convert|500|ly|pc|abbr=off|lk=on}} from Sun. The star is moving closer to the Earth with a heliocentric radial velocity of {{Val|−39|u=km/s}}, and may come as close as {{Convert|41.73|pc|ly|0|disp=out|abbr=off}} in around 3.5 million years.

The visible component is an A-type main sequence star with a stellar classification of A1 V. It has 3.25 times the mass of the Sun and about twice the Sun's radius. The projected rotational velocity is relatively low at 23 km/s. The star is radiating 214 times the luminosity of the Sun from its photosphere at an effective temperature of 9,908 K.

References

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}}