HD 183144

{{Short description|Suspected variable star in the constellation Aquila}}

{{Starbox begin

| name=HD 183144

}}

{{Starbox image

| image = 250px

| caption = A light curve for HD 183144, plotted from TESS data

}}

{{Starbox observe

| epoch = J2000

| constell = Aquila

| ra = {{RA|19|27|33.90756}}

| dec = {{DEC|+14|16|56.9284}}

| appmag_v = 6.32

}}

{{Starbox character

| class = B4III

| b-v = {{val|−0.068|0.005}}

| u-b = −0.512

| variable = suspected

}}

{{Starbox astrometry

| radial_v = {{val|+4.0|4.3}}

| prop_mo_ra = 6.162

| prop_mo_dec = −4.550

| parallax = 2.8745

| p_error = 0.0280

| parallax_footnote=

| absmag_v = −0.66

}}

{{Starbox detail

| mass = 5.1

| radius = 5.8

| luminosity = 2,676

| temperature = 15,139

| gravity = 3.73

| metal_fe = −0.003

| rotational_velocity=200

| age_myr = 160

}}

{{Starbox catalog

| names = {{odlist | BD=+13°4020 | HD=183144 | HIP=95664 | HR=7396 | SAO=104862 }}

}}

{{Starbox reference

| Simbad=HD+183144

}}

{{Starbox end}}

HD 183144 is a suspected variable star in the equatorial constellation of Aquila. It is a hot giant star about 1,130 light years away.

Results from the MASCARA experiment indicate that HD 183144 is a pulsating variable star with a period of 0.3649 days, during which it varies by 0.01 magnitude in white light. It has a mass five times that of the Sun and, at an age of 160 million years, has already evolved away from the main sequence. It has expended to nearly six times the radius of the Sun and, with an effective temperature of {{val|15,139|ul=K|fmt=commas}}, it has a bolometric luminosity of {{solar luminosity|2,676|link=y}}.

References

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}}